This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 08 05.4524 2461257.9524 12.48 05:49:28.36 +06:42:36.4
199.70535 -10.53294 galactic Ori Second-epoch detections are separated by 1.7" and 2.1 pix
The object was found in VSX 1" ASASSN-V J054928.37+064237.6
Type: L
# Max. Min./Amp. JD0 Period
13.730 V 14.070 V
The object was not found in astcheck.
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:49:28.36 +06:42:36.4: 13.47 +/- 0.03 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:49:28.36 +06:42:36.4: 13.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 05.4524* 05 49 28.36 +06 42 36.4 12.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J054928.37+064237.6,2461257.9524,12.48,0.05,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 J054928.37+064237.6 20260805.4524 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 05.4524 2461257.9524 12.37 05:53:21.83 +01:30:23.0
204.83539 -12.18387 galactic Ori Second-epoch detections are separated by 3.0" and 2.6 pix
The object was found in VSX 1" ASASSN-V J055321.79+013022.0
Type: L:
# Max. Min./Amp. JD0 Period
13.950 V 14.210 V
The object was not found in astcheck.
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:53:21.83 +01:30:23.0: 13.31 +/- 0.04 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:53:21.83 +01:30:23.0: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 05.4524* 05 53 21.83 +01 30 23.0 12.4 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 J055321.79+013022.0,2461257.9524,12.37,0.05,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 J055321.79+013022.0 20260805.4524 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 05.4524 2461257.9524 12.00 06:19:58.34 +02:34:04.9
207.03440 -5.81139 galactic Ori Second-epoch detections are separated by 1.4" and 2.0 pix
The object was found in VSX 6" NSVS J0619580+023401
Type: L:
# Max. Min./Amp. JD0 Period
11.045 R1 Y 0.500 R1 100.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:19:58.34 +02:34:04.9: 13.24 +/- 0.04 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:19:58.34 +02:34:04.9: 13.31 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 05.4524* 06 19 58.34 +02 34 04.9 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
NSVS J0619580+023401,2461257.9524,12.00,0.05,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 J0619580+023401 20260805.4524 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 05.4524 2461257.9524 12.14 06:17:37.29 +09:37:35.1
200.50349 -3.02376 galactic Ori Second-epoch detections are separated by 0.9" and 2.3 pix
The object was found in VSX 0" ASAS J061738+0937.5
Type: MISC
# Max. Min./Amp. JD0 Period
13.320 V Y 0.860 V 2452633.70000 187.400000000000 C
The object was not found in astcheck.
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:17:37.29 +09:37:35.1: 13.14 +/- 0.03 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:17:37.29 +09:37:35.1: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 05.4524* 06 17 37.29 +09 37 35.1 12.1 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 J061738+0937.5,2461257.9524,12.14,0.05,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 J061738+0937.5 20260805.4524 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 05.4524 2461257.9524 12.10 05:53:00.91 +02:42:39.1
203.70927 -11.68945 galactic Ori Second-epoch detections are separated by 0.6" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J088.2539+02.7104 | 05:53:00.94 +02:42:37.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=2.003+/-0.026 (Very red!)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:53:00.91 +02:42:39.1: 13.02 +/- 0.02 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:53:00.91 +02:42:39.1: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 05.4524* 05 53 00.91 +02 42 39.1 12.1 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
ATO J088.2539+02.7104,2461257.9524,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J088.2539+02.7104 20260805.4524 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 05.4524 2461257.9524 12.03 05:59:18.12 +07:54:31.0
199.84542 -7.82042 galactic Ori Second-epoch detections are separated by 0.7" and 2.0 pix
The object was found in VSX 0" ASAS J055918+0754.6
Type: MISC
# Max. Min./Amp. JD0 Period
13.130 V Y 0.710 V 2452495.90000 56.329620000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:59:18.12 +07:54:31.0: 13.00 +/- 0.02 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:59:18.12 +07:54:31.0: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 05.4524* 05 59 18.12 +07 54 31.0 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
ASAS J055918+0754.6,2461257.9524,12.03,0.05,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
ASAS J055918+0754.6 20260805.4524 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 08 05.4524 2461257.9524 11.82 06:15:19.20 +01:27:45.1
207.47847 -7.35366 galactic Ori Second-epoch detections are separated by 0.5" and 2.2 pix
The object was found in VSX 1" NSVS 12470304
Type: LPV
# Max. Min./Amp. JD0 Period
11.710 R1 Y 0.120 R1 84.880000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:15:19.20 +01:27:45.1: 12.93 +/- 0.03 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:15:19.20 +01:27:45.1: 12.88 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 05.4524* 06 15 19.20 +01 27 45.1 11.8 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
NSVS 12470304,2461257.9524,11.82,0.05,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 12470304 20260805.4524 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 05.4524 2461257.9524 11.89 06:07:20.88 +06:11:43.6
202.32622 -6.88961 galactic Ori Second-epoch detections are separated by 1.8" and 1.9 pix
The object was found in VSX 3" NSVS J0607211+061142
Type: L:
# Max. Min./Amp. JD0 Period
11.030 R1 Y 0.330 R1 157.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:07:20.88 +06:11:43.6: 12.79 +/- 0.02 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:07:20.88 +06:11:43.6: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 05.4524* 06 07 20.88 +06 11 43.6 11.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0607211+061142,2461257.9524,11.89,0.05,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 J0607211+061142 20260805.4524 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 05.4524 2461257.9524 12.73 05:56:58.50 +05:22:13.9
201.81313 -9.55028 galactic Ori Second-epoch detections are separated by 2.0" and 2.2 pix
The object was found in VSX 0" ASASSN-V J055658.51+052213.9
Type: SR
# Max. Min./Amp. JD0 Period
14.720 V 15.320 V 2457672.00000 61.100000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:56:58.50 +05:22:13.9: 14.14 +/- 0.06 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:56:58.50 +05:22:13.9: 14.21 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 05.4524* 05 56 58.50 +05 22 13.9 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 J055658.51+052213.9,2461257.9524,12.73,0.05,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 J055658.51+052213.9 20260805.4524 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 05.4524 2461257.9524 12.82 05:36:36.34 +04:30:15.1
200.06443 -14.40470 galactic Ori Second-epoch detections are separated by 2.2" and 2.0 pix
The object was found in VSX 1" ASASSN-V J053636.29+043014.5
Type: SR
# Max. Min./Amp. JD0 Period
15.640 g Y 0.990 g 2458702.67000 197.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:36:36.34 +04:30:15.1: 14.16 +/- 0.07 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:36:36.34 +04:30:15.1: 14.06 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 05.4524* 05 36 36.34 +04 30 15.1 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 J053636.29+043014.5,2461257.9524,12.82,0.05,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 J053636.29+043014.5 20260805.4524 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 05.4524 2461257.9524 12.49 06:06:03.62 +03:26:41.9
204.61837 -8.47336 galactic Ori Second-epoch detections are separated by 2.8" and 1.8 pix
The object was found in VSX 1" ASASSN-V J060603.69+032641.6
Type: L
# Max. Min./Amp. JD0 Period
14.010 V 14.650 V
The object was not found in astcheck.
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:06:03.62 +03:26:41.9: 14.03 +/- 0.06 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:06:03.62 +03:26:41.9: 14.01 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 05.4524* 06 06 03.62 +03 26 41.9 12.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J060603.69+032641.6,2461257.9524,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J060603.69+032641.6 20260805.4524 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 05.4524 2461257.9524 11.13 05:51:24.84 +04:18:19.5
202.08549 -11.27704 galactic Ori Second-epoch detections are separated by 0.6" and 2.2 pix
The object was found in VSX 0" ASAS J055125+0418.2
Type: MISC
# Max. Min./Amp. JD0 Period
12.660 V Y 0.940 V 2452648.60000 149.500000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:51:24.84 +04:18:19.5: 12.25 +/- 0.01 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:51:24.84 +04:18:19.5: 12.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 05.4524* 05 51 24.84 +04 18 19.5 11.1 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 J055125+0418.2,2461257.9524,11.13,0.05,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 J055125+0418.2 20260805.4524 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 05.4524 2461257.9524 10.79 06:19:37.22 +06:48:38.6
203.22594 -3.91157 galactic Ori Second-epoch detections are separated by 0.3" and 2.1 pix
The object was found in VSX 0" ASAS J061937+0648.7
Type: MISC
# Max. Min./Amp. JD0 Period
12.140 V Y 0.970 V 2453131.50000 415.000000000000 N
The object was not found in astcheck.
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:19:37.22 +06:48:38.6: 11.74 +/- 0.01 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:19:37.22 +06:48:38.6: 11.73 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 05.4524* 06 19 37.22 +06 48 38.6 10.8 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
ASAS J061937+0648.7,2461257.9524,10.79,0.05,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
ASAS J061937+0648.7 20260805.4524 10.79CV 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 08 05.4524 2461257.9524 12.75 05:44:21.58 +03:16:27.5
202.14173 -13.31585 galactic Ori Second-epoch detections are separated by 3.7" and 1.5 pix
The object was found in VSX 1" ASASSN-V J054421.55+031626.5
Type: SR
# Max. Min./Amp. JD0 Period
15.140 g Y 0.440 g 2459337.20400 59.050000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:44:21.58 +03:16:27.5: 13.81 +/- 0.05 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:44:21.58 +03:16:27.5: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 05.4524* 05 44 21.58 +03 16 27.5 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 J054421.55+031626.5,2461257.9524,12.75,0.05,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 J054421.55+031626.5 20260805.4524 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 05.4524 2461257.9524 9.54 06:02:10.96 +08:27:03.0
199.71397 -6.93433 galactic Ori Second-epoch detections are separated by 0.2" and 2.2 pix
The object was found in VSX 1" DR Ori
Type: LB
# Max. Min./Amp. JD0 Period
10.500 V Y 0.680 V 2452679.80000 135.007425000000 M6.5
The object was not found in astcheck.
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:02:10.96 +08:27:03.0: 10.52 +/- 0.00 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:02:10.96 +08:27:03.0: 10.50 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.51 +/- 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 08 05.4524* 06 02 10.96 +08 27 03.0 9.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DR Ori,2461257.9524,9.54,0.05,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
DR Ori 20260805.4524 9.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 05.4524 2461257.9524 12.63 05:52:45.97 +06:00:21.6
200.73548 -10.16084 galactic Ori Second-epoch detections are separated by 1.7" and 2.1 pix
The object was found in VSX 1" ASASSN-V J055246.01+060022.5
Type: SR
# Max. Min./Amp. JD0 Period
15.060 g Y 0.350 g 2458827.90700 31.030000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:52:45.97 +06:00:21.6: 13.75 +/- 0.04 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:52:45.97 +06:00:21.6: 13.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 05.4524* 05 52 45.97 +06 00 21.6 12.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J055246.01+060022.5,2461257.9524,12.63,0.05,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 J055246.01+060022.5 20260805.4524 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 05.4524 2461257.9524 12.48 05:58:50.51 +05:14:52.6
202.14800 -9.20126 galactic Ori Second-epoch detections are separated by 0.4" and 2.2 pix
The object was found in VSX 1" ASASSN-V J055850.45+051452.0
Type: SR
# Max. Min./Amp. JD0 Period
15.911 g Y 1.168 g 2458439.78930 181.054115000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:58:50.51 +05:14:52.6: 13.69 +/- 0.04 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:58:50.51 +05:14:52.6: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 05.4524* 05 58 50.51 +05 14 52.6 12.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J055850.45+051452.0,2461257.9524,12.48,0.05,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 J055850.45+051452.0 20260805.4524 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.61632350 11.02.2026 02:47:20.350 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
First image: 2461082.61632350 11.02.2026 02:47:20.350 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Last image: 2461257.95267604 05.08.2026 10:51:41.210 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 12
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.77
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 6 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): 22434
Objects passed selection criteria: 22300
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 14353.8
Average stars matched: 13895.8 (96.8092 %)
Memory usage VmPeak: 247044 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Aug 4 15:05:04 CDT 2026
VaST build number 1.0rc89-188-g9fc0b030
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-04)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Aug 5 05:55:53 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.61632350 11.02.2026 02:47:20.350 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
First image: 2461082.61632350 11.02.2026 02:47:20.350 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Last image: 2461257.95267604 05.08.2026 10:51:41.210 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 104
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.46
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 32 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): 150793
Objects passed selection criteria: 150312
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 98702
Average stars matched: 94797.5 (96.0442 %)
Memory usage VmPeak: 550228 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Aug 4 15:05:04 CDT 2026
VaST build number 1.0rc89-188-g9fc0b030
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-04)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Aug 5 05:57:18 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
SExtractor catalog cache: saved Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat to cache
SExtractor catalog cache: saved Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461257.95218976
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-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits exists and is non-empty
Saving wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits to local_wcs_cache/
'wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits' -> 'local_wcs_cache/wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits'
wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits exists and is non-empty
Saving wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits to local_wcs_cache/
'wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits' -> 'local_wcs_cache/wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits'
wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits exists and is non-empty
Saving wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits to local_wcs_cache/
'wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits' -> 'local_wcs_cache/wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits'
wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits exists and is non-empty
Saving wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits to local_wcs_cache/
'wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits' -> 'local_wcs_cache/wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits (1st reference image)
verification OK: wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Image size: 941.5'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:59:57.457 +05:59:33.15 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits (1st new image)
verification OK: wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
Image size: 944.6'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:00:00.260 +05:59:58.83 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:59:57.457 +05:59:33.15
Second-epoch image center 06:00:00.260 +05:59:58.83
Angular distance between the image centers 0.0136 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits (2nd new image)
verification OK: wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
Image size: 944.5'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:59:59.964 +05:59:47.01 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:59:57.457 +05:59:33.15
Second-epoch image center 05:59:59.964 +05:59:47.01
Angular distance between the image centers 0.0111 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 06:00:00.260 +05:59:58.83
Second-epoch second image center 05:59:59.964 +05:59:47.01
Angular distance between the image centers 0.00350 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits &> /tmp/tmp.hYlrYZycuF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits &> /tmp/tmp.nzkhjSeiz3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits &> /tmp/tmp.iuuA7oX21h
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits &> /tmp/tmp.VlwWvjOyUa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits and wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits and wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat
Found non-empty wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits and wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat
The reference image (wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits) and catalog (wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat) found
'wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat' -> 'wcsmag.cat'
Read 23947 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 81.9156 to 97.9251 deg, Dec +0.5852 to +11.3169 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 81.9156 to 97.9251 deg, Dec 0.5852 to 11.3169 deg
Loaded 13838 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 10471 out of 11616 total matches.
Matched with Tycho-2 11616 out of 23947 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.917600
a=0.000000 b=1.000000 c=22.917600
From vast_summary.log: estimated ref. image limiting mag.: -7.77
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.15
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.15
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 23947 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 81.9156 to 97.9251 deg, Dec +0.5852 to +11.3169 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 81.9156 to 97.9251 deg, Dec 0.5852 to 11.3169 deg
Loaded 13838 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 10471 out of 11616 total matches.
Matched with Tycho-2 11616 out of 23947 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Forced-photometry filter: calibrated wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits -> calib.txt_param_ref_wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits (aperture=6.3)
Read 23981 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 81.9156 to 97.9135 deg, Dec +0.6076 to +11.3239 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 81.9156 to 97.9135 deg, Dec 0.6076 to 11.3239 deg
Loaded 13821 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 10495 out of 11630 total matches.
Matched with Tycho-2 11630 out of 23981 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
Forced-photometry filter: calibrated wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits -> calib.txt_param_ref_wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 12 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
2.3 pix Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
3.3 pix fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
3.3 pix fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
Limiting magnitude estimates:
15.1 mag. Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
15.1 mag. Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
12.9 mag. fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
12.9 mag. fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
All-image limiting magnitude estimate: 12.9 (SNR ) 10.6 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.hYlrYZycuF (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits' -> 'wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
WCS_IMAGE_NAME=wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
WCS-calibrated image found: wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Checking if the catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat corresponding to the image wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits alredy exist and is non-empty...
Catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat corresponding to the image wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
WCS catalog name: wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2599, bad_region=0, passed=23947
Got 23947 stars (including 21319 good ones) from the SExtractor catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat
util/solve_plate_with_UCAC5 got 23947 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4843 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4781 matched stars entering correct_measured_positions(), 4781 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4781 matched stars entering correct_measured_positions(), 23947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4843 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4781 matched stars entering correct_measured_positions(), 23947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4781 matched stars entering correct_measured_positions(), 23947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4781 stars left (next iteration limit 5259)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits N_match=4781 sigma_overall_arcsec=0.442 sigma_q1_arcsec=0.485 sigma_q2_arcsec=0.402 sigma_q3_arcsec=0.393 sigma_q4_arcsec=0.445 n_q1=820 n_q2=1207 n_q3=1001 n_q4=1753 worst_quadrant_to_overall_ratio=1.098
The image catalog is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits -region wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.nzkhjSeiz3 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits' -> 'wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
WCS_IMAGE_NAME=wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
WCS-calibrated image found: wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
Checking if the catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat corresponding to the image wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits alredy exist and is non-empty...
Catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat corresponding to the image wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
WCS catalog name: wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2508, bad_region=0, passed=23981
Got 23981 stars (including 21438 good ones) from the SExtractor catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat
util/solve_plate_with_UCAC5 got 23981 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4842 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4781 matched stars entering correct_measured_positions(), 4781 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4781 matched stars entering correct_measured_positions(), 23981 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4842 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4780 matched stars entering correct_measured_positions(), 23981 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4780 matched stars entering correct_measured_positions(), 23981 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4780 stars left (next iteration limit 5259)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits N_match=4780 sigma_overall_arcsec=0.417 sigma_q1_arcsec=0.462 sigma_q2_arcsec=0.405 sigma_q3_arcsec=0.366 sigma_q4_arcsec=0.427 n_q1=829 n_q2=1201 n_q3=1010 n_q4=1740 worst_quadrant_to_overall_ratio=1.108
The image catalog is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits -region wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.iuuA7oX21h (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
WCS_IMAGE_NAME=wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
WCS-calibrated image found: wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
Checking if the catalog wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits.wcscat corresponding to the image wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits.wcscat corresponding to the image wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
WCS catalog name: wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.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=243, bad_region=0, passed=4900
Got 4900 stars (including 4655 good ones) from the SExtractor catalog wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits.wcscat
util/solve_plate_with_UCAC5 got 4900 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.6'
Seting catalog search parameters based on the expected field of view 944.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013119 (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 0.010496 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4481 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4403 matched stars entering correct_measured_positions(), 4403 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4403 matched stars entering correct_measured_positions(), 4897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4478 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4408 matched stars entering correct_measured_positions(), 4897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 4408 matched stars entering correct_measured_positions(), 4897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 4408 stars left (next iteration limit 4843)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4408 robust_rms=9.796 arcsec worst_quadrant_rms=12.914 arcsec
SIP_REFIT: SIP order 3 trial: matched=4408 robust_rms=0.561 arcsec worst_quadrant_rms=0.952 arcsec
SIP_REFIT: SIP order 5 trial: matched=4408 robust_rms=0.453 arcsec worst_quadrant_rms=0.632 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4408 robust_rms_before=1.455 arcsec robust_rms_before_corrected=0.492 arcsec robust_rms_after=0.453 arcsec worst_quadrant_rms_before=0.608 worst_quadrant_rms_after=0.632
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.608 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits N_match=4408 sigma_overall_arcsec=0.473 sigma_q1_arcsec=0.540 sigma_q2_arcsec=0.563 sigma_q3_arcsec=0.374 sigma_q4_arcsec=0.506 n_q1=1003 n_q2=658 n_q3=1360 n_q4=1387 worst_quadrant_to_overall_ratio=1.190
The image catalog is written to wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits -region wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.VlwWvjOyUa (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
WCS_IMAGE_NAME=wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
WCS-calibrated image found: wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
Checking if the catalog wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits.wcscat corresponding to the image wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits.wcscat corresponding to the image wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
WCS catalog name: wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.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=248, bad_region=0, passed=4946
Got 4946 stars (including 4693 good ones) from the SExtractor catalog wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits.wcscat
util/solve_plate_with_UCAC5 got 4946 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.5'
Seting catalog search parameters based on the expected field of view 944.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013118 (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 0.010494 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4519 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4443 matched stars entering correct_measured_positions(), 4444 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4443 matched stars entering correct_measured_positions(), 4945 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 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4513 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4444 matched stars entering correct_measured_positions(), 4945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 4444 matched stars entering correct_measured_positions(), 4945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 4444 stars left (next iteration limit 4887)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4444 robust_rms=10.004 arcsec worst_quadrant_rms=12.869 arcsec
SIP_REFIT: SIP order 3 trial: matched=4444 robust_rms=0.550 arcsec worst_quadrant_rms=0.837 arcsec
SIP_REFIT: SIP order 5 trial: matched=4444 robust_rms=0.451 arcsec worst_quadrant_rms=0.712 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4444 robust_rms_before=1.367 arcsec robust_rms_before_corrected=0.498 arcsec robust_rms_after=0.451 arcsec worst_quadrant_rms_before=0.607 worst_quadrant_rms_after=0.712
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.607 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits N_match=4444 sigma_overall_arcsec=0.487 sigma_q1_arcsec=0.529 sigma_q2_arcsec=0.584 sigma_q3_arcsec=0.395 sigma_q4_arcsec=0.540 n_q1=1004 n_q2=666 n_q3=1373 n_q4=1401 worst_quadrant_to_overall_ratio=1.199
The image catalog is written to wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits -region wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits sigma_overall=0.442 worst_q_ratio=1.098
ref2=Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits sigma_overall=0.417 worst_q_ratio=1.108
new1=fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits sigma_overall=0.473 worst_q_ratio=1.190
new2=fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits sigma_overall=0.487 worst_q_ratio=1.199
reference average sigma_overall=0.4295 worst_q_ratio=1.103
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032_astrometric_residuals.png (4781 matched stars from wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033_astrometric_residuals.png (4780 matched stars from wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.38 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482_astrometric_residuals.png (4408 matched stars from wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.44 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483_astrometric_residuals.png (4444 matched stars from wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.45 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits'
Saving fully-calibrated image wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits'
Preparing the HTML report for the field Ori-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31607_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 31607_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:15:59.66 +10:33:40.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31608_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 31608_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:08:59.72 +02:29:46.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31707_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 31707_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:44:28.85 +06:52:01.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31736_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 31736_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:55:04.21 +07:30:08.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10971_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 10971_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:01:48.28 +06:38:19.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13836_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 13836_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:31:56.01 +07:36:48.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05113_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 05113_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:10:44.97 +03:45:24.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10180_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 10180_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:06:03.51 +06:19:12.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02948_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 02948_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:46:27.38 +02:18:31.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01005_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 01005_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:52:45.15 +01:13:22.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16466_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 16466_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:02:43.46 +08:42:04.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06293_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 06293_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:23:45.99 +04:35:35.4 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Ori-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
SExtractor catalog cache: saved Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat to cache
SExtractor catalog cache: saved Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Creating symlink local_wcs_cache/wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits exists and is non-empty
wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits exists and is non-empty
wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits exists and is non-empty
wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits (1st reference image)
verification OK: wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Image size: 941.5'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:59:57.457 +05:59:33.15 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits (1st new image)
verification OK: wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
Image size: 944.6'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:00:00.260 +05:59:58.83 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:59:57.457 +05:59:33.15
Second-epoch image center 06:00:00.260 +05:59:58.83
Angular distance between the image centers 0.0136 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits (2nd new image)
verification OK: wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
Image size: 944.5'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:59:59.964 +05:59:47.01 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:59:57.457 +05:59:33.15
Second-epoch image center 05:59:59.964 +05:59:47.01
Angular distance between the image centers 0.0111 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 06:00:00.260 +05:59:58.83
Second-epoch second image center 05:59:59.964 +05:59:47.01
Angular distance between the image centers 0.00350 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits &> /tmp/tmp.iEvpmVI6DN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits &> /tmp/tmp.6eYcIUCCVF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits &> /tmp/tmp.E0LhH83CJe
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits &> /tmp/tmp.mpzGzCZAMx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits and wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits and wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat
Found non-empty wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits and wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat
The reference image (wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits) and catalog (wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat) found
'wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat' -> 'wcsmag.cat'
Read 165923 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 81.9025 to 97.9258 deg, Dec +0.5713 to +11.3193 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 81.9025 to 97.9258 deg, Dec 0.5713 to 11.3193 deg
Loaded 13864 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 8480 out of 12115 total matches.
Matched with Tycho-2 12115 out of 165923 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.768800
a=0.000000 b=1.000000 c=22.768800
From vast_summary.log: estimated ref. image limiting mag.: -7.46
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 165923 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 81.9025 to 97.9258 deg, Dec +0.5713 to +11.3193 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 81.9025 to 97.9258 deg, Dec 0.5713 to 11.3193 deg
Loaded 13864 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 8480 out of 12115 total matches.
Matched with Tycho-2 12115 out of 165923 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Forced-photometry filter: calibrated wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits -> calib.txt_param_ref_wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits (aperture=4.7)
Read 164824 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 81.8906 to 97.9164 deg, Dec +0.5830 to +11.3271 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 81.8906 to 97.9164 deg, Dec 0.5830 to 11.3271 deg
Loaded 13866 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 8525 out of 12126 total matches.
Matched with Tycho-2 12126 out of 164824 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
Forced-photometry filter: calibrated wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits -> calib.txt_param_ref_wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 100 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
2.1 pix Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
3.1 pix fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
3.0 pix fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
Limiting magnitude estimates:
15.3 mag. Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
15.3 mag. Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
13.1 mag. fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
13.2 mag. fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
All-image limiting magnitude estimate: 13.1 (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.iEvpmVI6DN (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits' -> 'wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
WCS_IMAGE_NAME=wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
WCS-calibrated image found: wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Checking if the catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat corresponding to the image wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits alredy exist and is non-empty...
Catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat corresponding to the image wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
WCS catalog name: wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=50, blended=21856, bad_region=0, passed=165873
Got 165873 stars (including 143783 good ones) from the SExtractor catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat
util/solve_plate_with_UCAC5 got 165873 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4836 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4784 matched stars entering correct_measured_positions(), 4785 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4784 matched stars entering correct_measured_positions(), 165873 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4836 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4786 matched stars entering correct_measured_positions(), 165873 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4786 matched stars entering correct_measured_positions(), 165873 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 4786 stars left (next iteration limit 5262)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits N_match=4786 sigma_overall_arcsec=0.403 sigma_q1_arcsec=0.436 sigma_q2_arcsec=0.383 sigma_q3_arcsec=0.361 sigma_q4_arcsec=0.418 n_q1=899 n_q2=1223 n_q3=1055 n_q4=1609 worst_quadrant_to_overall_ratio=1.083
The image catalog is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits -region wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.6eYcIUCCVF (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits' -> 'wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
WCS_IMAGE_NAME=wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
WCS-calibrated image found: wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
Checking if the catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat corresponding to the image wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits alredy exist and is non-empty...
Catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat corresponding to the image wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
WCS catalog name: wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=53, blended=21523, bad_region=1, passed=164771
Got 164771 stars (including 143000 good ones) from the SExtractor catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat
util/solve_plate_with_UCAC5 got 164771 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4841 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4795 matched stars entering correct_measured_positions(), 4795 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4795 matched stars entering correct_measured_positions(), 164771 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4841 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4794 matched stars entering correct_measured_positions(), 164771 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4794 matched stars entering correct_measured_positions(), 164771 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 4794 stars left (next iteration limit 5274)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits N_match=4794 sigma_overall_arcsec=0.399 sigma_q1_arcsec=0.413 sigma_q2_arcsec=0.375 sigma_q3_arcsec=0.348 sigma_q4_arcsec=0.422 n_q1=916 n_q2=1211 n_q3=1057 n_q4=1610 worst_quadrant_to_overall_ratio=1.056
The image catalog is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits -region wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.E0LhH83CJe (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
WCS_IMAGE_NAME=wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
WCS-calibrated image found: wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
Checking if the catalog wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits.wcscat corresponding to the image wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits.wcscat corresponding to the image wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
WCS catalog name: wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.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=3, blended=1176, bad_region=2, passed=33150
Got 33150 stars (including 31939 good ones) from the SExtractor catalog wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits.wcscat
util/solve_plate_with_UCAC5 got 33150 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.6'
Seting catalog search parameters based on the expected field of view 944.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013119 (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 0.010496 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4809 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4727 matched stars entering correct_measured_positions(), 4732 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4727 matched stars entering correct_measured_positions(), 33141 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4806 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4732 matched stars entering correct_measured_positions(), 33139 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 4732 matched stars entering correct_measured_positions(), 33139 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 4732 stars left (next iteration limit 5199)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits N_match=4732 sigma_overall_arcsec=0.498 sigma_q1_arcsec=0.555 sigma_q2_arcsec=0.573 sigma_q3_arcsec=0.397 sigma_q4_arcsec=0.553 n_q1=1067 n_q2=696 n_q3=1507 n_q4=1462 worst_quadrant_to_overall_ratio=1.150
The image catalog is written to wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits -region wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.mpzGzCZAMx (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
WCS_IMAGE_NAME=wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
WCS-calibrated image found: wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
Checking if the catalog wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits.wcscat corresponding to the image wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits.wcscat corresponding to the image wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
WCS catalog name: wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.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=6, blended=1142, bad_region=3, passed=33344
Got 33344 stars (including 32162 good ones) from the SExtractor catalog wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits.wcscat
util/solve_plate_with_UCAC5 got 33344 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.5'
Seting catalog search parameters based on the expected field of view 944.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013118 (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 0.010494 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4810 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(), 4735 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4731 matched stars entering correct_measured_positions(), 33338 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 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4804 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4732 matched stars entering correct_measured_positions(), 33338 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 4732 matched stars entering correct_measured_positions(), 33338 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 4732 stars left (next iteration limit 5204)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits N_match=4732 sigma_overall_arcsec=0.486 sigma_q1_arcsec=0.511 sigma_q2_arcsec=0.579 sigma_q3_arcsec=0.383 sigma_q4_arcsec=0.539 n_q1=1046 n_q2=713 n_q3=1499 n_q4=1474 worst_quadrant_to_overall_ratio=1.192
The image catalog is written to wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits -region wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-50-59_20.00sec_-0.00C_LIGHTs_0482.fits
Saving fully-calibrated image wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_Ori-04-Q1b1x1_055315_TTUQ1b1x1_1112381_Ef51ZKRD/wcs_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483.fits
Preparing the HTML report for the field Ori-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:20:46.50 +00:49:01.2: 99.00 +/- 99.00 edge
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:07:21.32 +09:10:48.7: 12.35 +/- 0.02 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:07:21.32 +09:10:48.7: 12.36 +/- 0.02 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:20:46.50 +00:49:01.2: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 06:20:46.50 +00:49:01.2: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Forced photometry filter REJECTED candidate at 06:07:21.32 +09:10:48.7: ref_mag=12.35 +/- 0.01 new_mean_mag=12.1529 delta=0.20 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:53:21.83 +01:30:23.0: 13.31 +/- 0.04 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:49:28.36 +06:42:36.4: 13.47 +/- 0.03 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:19:58.34 +02:34:04.9: 13.24 +/- 0.04 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:53:21.83 +01:30:23.0: 13.27 +/- 0.04 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:49:28.36 +06:42:36.4: 13.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.03
Forced photometry filter KEPT candidate at 05:53:21.83 +01:30:23.0: ref_mag=13.29 +/- 0.03 new_mean_mag=12.3422 delta=0.95 (need > 0.90)
Forced photometry reference-image weighted average: 13.44 +/- 0.02
Forced photometry filter KEPT candidate at 05:49:28.36 +06:42:36.4: ref_mag=13.44 +/- 0.02 new_mean_mag=12.4786 delta=0.96 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:19:58.34 +02:34:04.9: 13.31 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Forced photometry filter KEPT candidate at 06:19:58.34 +02:34:04.9: ref_mag=13.27 +/- 0.03 new_mean_mag=11.9934 delta=1.28 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:17:37.29 +09:37:35.1: 13.14 +/- 0.03 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:59:18.12 +07:54:31.0: 13.00 +/- 0.02 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:53:00.91 +02:42:39.1: 13.02 +/- 0.02 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:17:37.29 +09:37:35.1: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry filter KEPT candidate at 06:17:37.29 +09:37:35.1: ref_mag=13.13 +/- 0.02 new_mean_mag=12.1457 delta=0.99 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:59:18.12 +07:54:31.0: 12.98 +/- 0.02 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:53:00.91 +02:42:39.1: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Forced photometry filter KEPT candidate at 05:59:18.12 +07:54:31.0: ref_mag=12.99 +/- 0.02 new_mean_mag=12.0299 delta=0.96 (need > 0.90)
Forced photometry filter KEPT candidate at 05:53:00.91 +02:42:39.1: ref_mag=13.01 +/- 0.02 new_mean_mag=12.0932 delta=0.92 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:15:19.20 +01:27:45.1: 12.93 +/- 0.03 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:07:20.88 +06:11:43.6: 12.79 +/- 0.02 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:15:19.20 +01:27:45.1: 12.88 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Forced photometry filter KEPT candidate at 06:15:19.20 +01:27:45.1: ref_mag=12.90 +/- 0.02 new_mean_mag=11.8284 delta=1.07 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:07:20.88 +06:11:43.6: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Forced photometry filter KEPT candidate at 06:07:20.88 +06:11:43.6: ref_mag=12.78 +/- 0.01 new_mean_mag=11.8773 delta=0.91 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:56:58.50 +05:22:13.9: 14.14 +/- 0.06 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:56:58.50 +05:22:13.9: 14.21 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.04
Forced photometry filter KEPT candidate at 05:56:58.50 +05:22:13.9: ref_mag=14.17 +/- 0.04 new_mean_mag=12.7179 delta=1.46 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:36:36.34 +04:30:15.1: 14.16 +/- 0.07 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:36:36.34 +04:30:15.1: 14.06 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.05
Forced photometry filter KEPT candidate at 05:36:36.34 +04:30:15.1: ref_mag=14.10 +/- 0.05 new_mean_mag=12.8155 delta=1.29 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:27:48.78 +06:06:27.7: 12.48 +/- 0.02 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:06:03.62 +03:26:41.9: 14.03 +/- 0.06 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:27:48.78 +06:06:27.7: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Forced photometry filter REJECTED candidate at 06:27:48.78 +06:06:27.7: ref_mag=12.49 +/- 0.01 new_mean_mag=11.6691 delta=0.82 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:51:24.84 +04:18:19.5: 12.25 +/- 0.01 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:06:03.62 +03:26:41.9: 14.01 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.04
Forced photometry filter KEPT candidate at 06:06:03.62 +03:26:41.9: ref_mag=14.02 +/- 0.04 new_mean_mag=12.4856 delta=1.54 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:51:24.84 +04:18:19.5: 12.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Forced photometry filter KEPT candidate at 05:51:24.84 +04:18:19.5: ref_mag=12.24 +/- 0.01 new_mean_mag=11.1306 delta=1.11 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:19:37.22 +06:48:38.6: 11.74 +/- 0.01 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:44:21.58 +03:16:27.5: 13.81 +/- 0.05 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:19:37.22 +06:48:38.6: 11.73 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.73 +/- 0.01
Forced photometry filter KEPT candidate at 06:19:37.22 +06:48:38.6: ref_mag=11.73 +/- 0.01 new_mean_mag=10.7803 delta=0.95 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:44:21.58 +03:16:27.5: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Forced photometry filter KEPT candidate at 05:44:21.58 +03:16:27.5: ref_mag=13.81 +/- 0.03 new_mean_mag=12.7482 delta=1.06 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:02:10.96 +08:27:03.0: 10.52 +/- 0.00 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:52:45.97 +06:00:21.6: 13.75 +/- 0.04 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:02:10.96 +08:27:03.0: 10.50 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.51 +/- 0.00
Forced photometry filter KEPT candidate at 06:02:10.96 +08:27:03.0: ref_mag=10.51 +/- 0.00 new_mean_mag=9.5399 delta=0.97 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:58:50.51 +05:14:52.6: 13.69 +/- 0.04 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:52:45.97 +06:00:21.6: 13.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.03
Forced photometry filter KEPT candidate at 05:52:45.97 +06:00:21.6: ref_mag=13.78 +/- 0.03 new_mean_mag=12.6228 delta=1.15 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:58:50.51 +05:14:52.6: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Forced photometry filter KEPT candidate at 05:58:50.51 +05:14:52.6: ref_mag=13.70 +/- 0.03 new_mean_mag=12.4729 delta=1.23 (need > 0.90)
Adding exclusion_list_local.txt__out07897.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09677.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out101866.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114259.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131416.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20895.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23680.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30762.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43889.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56015.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58196.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68478.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70757.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80695.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80696.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
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: 9s
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Considering the candidate 190090_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190090_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:52:13.80 +09:13:19.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190099_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190099_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:00:48.65 +08:35:09.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190102_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190102_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:52:20.61 +07:17:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190104_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190104_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:22:12.78 +09:54:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190109_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190109_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:20:00.90 +10:43:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190111_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190111_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:15:59.63 +10:33:39.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190135_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190135_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:31:30.95 +09:13:02.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 190294_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190294_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 190322_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190322_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:54:56.04 +07:25:55.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 190324_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190324_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 190343_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190343_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 190376_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190376_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:48:01.31 +06:28:46.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 190439_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190439_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 190530_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190530_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 190550_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190550_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:30:24.52 +04:10:59.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 190643_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190643_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:35:55.96 +09:31:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190685_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190685_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 190747_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190747_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 190786_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190786_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:23:53.60 +04:36:12.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 190818_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190818_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:43:24.07 +10:29:54.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190827_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190827_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:36:59.95 +09:15:23.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 190830_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190830_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
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Considering the candidate 190834_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190834_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
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Considering the candidate 190858_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190858_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:37:13.38 +08:14:00.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190892_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190892_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:39:33.34 +09:52:21.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190905_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190905_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 190906_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190906_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 190931_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190931_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:42:19.76 +02:19:43.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190936_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190936_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:54:16.49 +10:33:28.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 190939_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190939_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:07:10.11 +09:11:16.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190943_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190943_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:06:23.11 +10:45:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190992_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 190992_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:11:16.58 +08:30:28.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191108_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 191108_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:44:09.04 +09:09:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191226_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 191226_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 191253_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 191253_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:50:22.14 +02:02:57.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191256_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 191256_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:04:22.12 +06:35:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191257_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 191257_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 191293_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 191293_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 189385_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 189385_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 111548_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 111548_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:12:45.85 +08:27:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81101_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 81101_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:46:42.05 +06:43:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80696_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
Preparing report for the candidate 80696_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
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Considering the candidate 45229_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 45229_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:47:51.53 +04:25:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 135524_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 135524_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:18:56.10 +09:18:19.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 09677_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
Preparing report for the candidate 09677_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
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Considering the candidate 20895_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
Preparing report for the candidate 20895_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
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Considering the candidate 23194_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 23194_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:55:09.31 +02:40:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 131416_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
Preparing report for the candidate 131416_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
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Considering the candidate 155457_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 155457_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:18:03.49 +10:31:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 140915_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 140915_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:15:34.88 +08:57:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 42580_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 42580_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:29:10.17 +04:23:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23680_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
Preparing report for the candidate 23680_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
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Considering the candidate 101866_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
Preparing report for the candidate 101866_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
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Considering the candidate 132306_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 132306_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:02:49.64 +09:32:10.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07897_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
Preparing report for the candidate 07897_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
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Considering the candidate 18414_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 18414_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:12:59.38 +02:20:47.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70757_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
Preparing report for the candidate 70757_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
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Considering the candidate 84127_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 84127_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:44:28.86 +06:52:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157497_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 157497_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:26:52.52 +10:23:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58196_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
Preparing report for the candidate 58196_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
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Considering the candidate 46973_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
Preparing report for the candidate 46973_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
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Considering the candidate 40658_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 40658_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:52:20.77 +04:05:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129238_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 129238_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:45:43.61 +09:35:34.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64338_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 64338_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:06:40.97 +05:44:54.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 68436_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 68436_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
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Considering the candidate 108481_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 108481_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:13:52.12 +08:15:10.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23509_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 23509_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 89762_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 89762_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:07:20.12 +07:14:26.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 46740_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 46740_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:06:06.72 +04:35:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31538_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
Preparing report for the candidate 31538_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
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Considering the candidate 22762_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 22762_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:44:36.75 +02:36:42.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79997_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 79997_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:16:06.36 +06:46:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 43889_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
Preparing report for the candidate 43889_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
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Considering the candidate 20875_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 20875_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:17:07.39 +02:34:45.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127054_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 127054_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:23:18.35 +09:50:37.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93094_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 93094_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:11:19.26 +07:28:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23768_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 23768_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:57:28.35 +02:46:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 143663_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 143663_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:02:43.44 +08:42:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51689_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 51689_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:23:11.87 +05:00:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112160_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 112160_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:05:09.07 +08:25:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80695_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
Preparing report for the candidate 80695_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
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Considering the candidate 102420_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 102420_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:31:56.02 +07:36:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30762_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
Preparing report for the candidate 30762_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
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Considering the candidate 07744_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 07744_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:38:47.88 +01:16:39.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33592_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 33592_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:10:44.97 +03:45:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78868_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 78868_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:01:48.28 +06:38:19.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18787_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 18787_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:46:27.39 +02:18:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73780_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 73780_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:06:03.51 +06:19:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114259_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
Preparing report for the candidate 114259_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
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Considering the candidate 05061_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 05061_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:52:45.16 +01:13:22.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69814_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 69814_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:57:29.61 +06:06:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 68478_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
Preparing report for the candidate 68478_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
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Considering the candidate 56015_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
Preparing report for the candidate 56015_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
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Considering the candidate 60465_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 60465_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:04:58.06 +05:25:09.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 41851_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 41851_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:04:58.26 +04:09:31.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 19427_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 19427_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:08:58.06 +02:29:57.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 12333_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 12333_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 05:52:26.59 +01:51:20.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 54433_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 54433_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:17:15.66 +05:06:03.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 23134_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 23134_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
**** FOUND 06:27:20.32 +02:54:29.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 46896_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483
The candidate 46896_fd_Ori-04-Q1b1x1_2026-08-05_05-51-41_20.00sec_-0.00C_LIGHTs_0483 did not pass the final checks
