This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 07 10.3489 2461231.8489 11.01 00:25:41.97 +27:46:14.9
115.99989 -34.75427 galactic And Second-epoch detections are separated by 1.1" and 7.0 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 | Gaia DR3 2856261180073924992 | 00:25:41.94 +27:46:15.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.682+/-0.030 (K)
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:25:41.97 +27:46:14.9: 12.07 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:25:41.97 +27:46:14.9: 12.09 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3489* 00 25 41.97 +27 46 14.9 11.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2856261180073924992,2461231.8489,11.01,0.05,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
Gaia DR3 2856261180073924992 20260710.3489 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3489 2461231.8489 10.63 00:26:17.80 +34:20:14.6
117.04181 -28.24666 galactic And Second-epoch detections are separated by 1.7" and 6.4 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 | Large-amplitude variable Gaia DR2 2863927318740364672 | 00:26:17.74 +34:20:14.9 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: F6 (LAMOST DR5) J-Ks=0.291+/-0.027 (F)
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:26:17.80 +34:20:14.6: 11.56 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:26:17.80 +34:20:14.6: 11.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.58 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3489* 00 26 17.80 +34 20 14.6 10.6 U And 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
Large-amplitude variable Gaia DR2 2863927318740364672,2461231.8489,10.63,0.05,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
Large-amplitude variable Gaia DR2 2863927318740364672 20260710.3489 10.63CV 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 07 10.3489 2461231.8489 10.86 00:35:36.70 +34:51:05.1
119.25813 -27.90741 galactic And Second-epoch detections are separated by 0.7" and 6.6 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 | Gaia DR3 365259141432515840 | 00:35:36.71 +34:51:04.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F3 (LAMOST DR5) J-Ks=0.251+/-0.027 (F)
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:35:36.70 +34:51:05.1: 11.86 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:35:36.70 +34:51:05.1: 11.89 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.87 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3489* 00 35 36.70 +34 51 05.1 10.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 365259141432515840,2461231.8489,10.86,0.05,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
Gaia DR3 365259141432515840 20260710.3489 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3489 2461231.8489 11.27 00:36:09.04 +29:07:33.1
118.92212 -33.62684 galactic And Second-epoch detections are separated by 3.6" and 6.6 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 | Gaia DR3 2857811525828872576 | 00:36:08.95 +29:07:33.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.726+/-0.031 (K)
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:36:09.04 +29:07:33.1: 12.30 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:36:09.04 +29:07:33.1: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3489* 00 36 09.04 +29 07 33.1 11.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2857811525828872576,2461231.8489,11.27,0.05,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
Gaia DR3 2857811525828872576 20260710.3489 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3489 2461231.8489 11.13 00:25:41.96 +34:07:00.7
116.87432 -28.45197 galactic And Second-epoch detections are separated by 1.6" and 6.7 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 | Gaia DR3 2863897838084761600 | 00:25:42.00 +34:07:00.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5) J-Ks=0.356+/-0.028 (G)
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:25:41.96 +34:07:00.7: 12.27 +/- 0.02 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:25:41.96 +34:07:00.7: 12.29 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3489* 00 25 41.96 +34 07 00.7 11.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2863897838084761600,2461231.8489,11.13,0.05,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
Gaia DR3 2863897838084761600 20260710.3489 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 07 10.3489 2461231.8489 10.62 00:25:12.88 +27:43:51.8
115.86437 -34.78057 galactic And Second-epoch detections are separated by 5.1" and 6.8 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 | Gaia DR3 2856260458520039552 | 00:25:13.06 +27:43:53.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:25:12.88 +27:43:51.8: 11.60 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:25:12.88 +27:43:51.8: 11.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.62 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3489* 00 25 12.88 +27 43 51.8 10.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2856260458520039552,2461231.8489,10.62,0.05,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
Gaia DR3 2856260458520039552 20260710.3489 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3489 2461231.8489 10.70 00:26:14.45 +34:21:12.1
117.03081 -28.22951 galactic And Second-epoch detections are separated by 0.7" and 6.7 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 | Gaia DR3 2863933396118297344 | 00:26:14.46 +34:21:11.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.584+/-0.027 (K)
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:26:14.45 +34:21:12.1: 11.69 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:26:14.45 +34:21:12.1: 11.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3489* 00 26 14.45 +34 21 12.1 10.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2863933396118297344,2461231.8489,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2863933396118297344 20260710.3489 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3489 2461231.8489 11.14 00:36:10.48 +29:23:37.7
118.95122 -33.35994 galactic And Second-epoch detections are separated by 0.9" and 6.7 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 | Gaia DR3 2858007475121662848 | 00:36:10.52 +29:23:38.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.501+/-0.032 (K)
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:36:10.48 +29:23:37.7: 12.16 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:36:10.48 +29:23:37.7: 12.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3489* 00 36 10.48 +29 23 37.7 11.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2858007475121662848,2461231.8489,11.14,0.05,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
Gaia DR3 2858007475121662848 20260710.3489 11.14CV 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 07 10.3489 2461231.8489 11.23 00:36:16.94 +34:44:34.7
119.40530 -28.02498 galactic And Second-epoch detections are separated by 1.6" and 6.4 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 | Gaia DR3 365068891561215232 | 00:36:16.89 +34:44:35.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8 (LAMOST DR5) J-Ks=0.476+/-0.030 (K)
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:36:16.94 +34:44:34.7: 12.13 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:36:16.94 +34:44:34.7: 12.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3489* 00 36 16.94 +34 44 34.7 11.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 365068891561215232,2461231.8489,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 365068891561215232 20260710.3489 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3489 2461231.8489 11.18 00:53:51.65 +34:31:20.0
123.49898 -28.34686 galactic And Second-epoch detections are separated by 1.2" and 6.6 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 | Gaia DR3 362940026595767680 | 00:53:51.62 +34:31:20.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.618+/-0.029 (K)
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:53:51.65 +34:31:20.0: 12.11 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:53:51.65 +34:31:20.0: 12.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3489* 00 53 51.65 +34 31 20.0 11.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 362940026595767680,2461231.8489,11.18,0.05,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
Gaia DR3 362940026595767680 20260710.3489 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3489 2461231.8489 10.57 00:25:55.41 +34:13:09.0
116.93983 -28.35555 galactic And Second-epoch detections are separated by 0.1" and 6.7 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 | Gaia DR3 2863925016637902720 | 00:25:55.43 +34:13:08.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.306+/-0.027 (F)
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:25:55.41 +34:13:09.0: 11.57 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:25:55.41 +34:13:09.0: 11.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3489* 00 25 55.41 +34 13 09.0 10.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2863925016637902720,2461231.8489,10.57,0.05,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
Gaia DR3 2863925016637902720 20260710.3489 10.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3489 2461231.8489 10.56 00:35:47.38 +34:49:12.8
119.29693 -27.94106 galactic And Second-epoch detections are separated by 0.4" and 6.4 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 | Gaia DR3 365258076280629504 | 00:35:47.34 +34:49:13.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0 (LAMOST DR5) J-Ks=0.942+/-0.032 (M)
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:35:47.38 +34:49:12.8: 11.50 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:35:47.38 +34:49:12.8: 11.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.51 +/- 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 07 10.3489* 00 35 47.38 +34 49 12.8 10.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 365258076280629504,2461231.8489,10.56,0.05,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
Gaia DR3 365258076280629504 20260710.3489 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3489 2461231.8489 10.54 00:33:48.29 +31:17:59.0
118.51795 -31.42086 galactic And Second-epoch detections are separated by 1.5" and 6.8 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 | Gaia DR3 2859362249540745472 | 00:33:48.29 +31:17:58.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.321+/-0.034 (F)
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:33:48.29 +31:17:59.0: 11.47 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:33:48.29 +31:17:59.0: 11.48 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.48 +/- 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 07 10.3489* 00 33 48.29 +31 17 59.0 10.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2859362249540745472,2461231.8489,10.54,0.05,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
Gaia DR3 2859362249540745472 20260710.3489 10.54CV 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 07 10.3489 2461231.8489 10.55 00:35:43.32 +34:49:15.6
119.28131 -27.93932 galactic And Second-epoch detections are separated by 0.4" and 6.5 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 | Gaia DR3 365258110640367616 | 00:35:43.29 +34:49:15.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.389+/-0.026 (G)
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:35:43.32 +34:49:15.6: 11.45 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:35:43.32 +34:49:15.6: 11.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.47 +/- 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 07 10.3489* 00 35 43.32 +34 49 15.6 10.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 365258110640367616,2461231.8489,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 365258110640367616 20260710.3489 10.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3489 2461231.8489 10.96 00:35:22.09 +34:58:08.6
119.21112 -27.78657 galactic And Second-epoch detections are separated by 1.7" and 6.6 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 | Gaia DR3 365263711277706496 | 00:35:23.83 +34:58:48.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.726+/-0.028 (K)
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:35:22.09 +34:58:08.6: 12.01 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:35:22.09 +34:58:08.6: 12.02 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3489* 00 35 22.09 +34 58 08.6 11.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 365263711277706496,2461231.8489,10.96,0.05,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
Gaia DR3 365263711277706496 20260710.3489 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3489 2461231.8489 11.04 00:36:31.42 +29:21:37.4
119.03924 -33.39861 galactic And Second-epoch detections are separated by 1.1" and 6.7 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 | Gaia DR3 2858378697734382848 | 00:36:31.40 +29:21:37.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.309+/-0.031 (F)
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:36:31.42 +29:21:37.4: 12.01 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:36:31.42 +29:21:37.4: 12.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.04 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3489* 00 36 31.42 +29 21 37.4 11.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2858378697734382848,2461231.8489,11.04,0.05,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
Gaia DR3 2858378697734382848 20260710.3489 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3489 2461231.8489 10.97 00:36:13.65 +34:54:04.5
119.40454 -27.86630 galactic And Second-epoch detections are separated by 1.8" and 6.7 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 | Gaia DR3 365260069145450752 | 00:36:13.67 +34:54:03.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.634+/-0.028 (K)
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:36:13.65 +34:54:04.5: 11.91 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:36:13.65 +34:54:04.5: 11.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.93 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3489* 00 36 13.65 +34 54 04.5 11.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 365260069145450752,2461231.8489,10.97,0.05,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
Gaia DR3 365260069145450752 20260710.3489 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3489 2461231.8489 10.71 00:25:34.61 +34:13:04.3
116.85875 -28.34874 galactic And Second-epoch detections are separated by 1.0" and 6.7 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 | Gaia DR3 2863925562097955072 | 00:25:34.55 +34:13:04.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.172+/-0.028 (F)
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:25:34.61 +34:13:04.3: 11.90 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:25:34.61 +34:13:04.3: 11.93 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3489* 00 25 34.61 +34 13 04.3 10.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2863925562097955072,2461231.8489,10.71,0.05,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
Gaia DR3 2863925562097955072 20260710.3489 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.68993344 23.12.2025 04:33:20.249 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
First image: 2461032.68993344 23.12.2025 04:33:20.249 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
Last image: 2461231.85002420 10.07.2026 08:23:52.091 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.55
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 11053
Objects passed selection criteria: 10946
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 4
Average stars detected per image: 6103.75
Average stars matched: 6005.75 (98.3944 %)
Memory usage VmPeak: 116768 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 8 15:05:08 CDT 2026
VaST build number 1.0rc89-141-gc31ee76a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 10 06:56:43 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: 2461032.68993344 23.12.2025 04:33:20.249 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
First image: 2461032.68993344 23.12.2025 04:33:20.249 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
Last image: 2461231.85002420 10.07.2026 08:23:52.091 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 29
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.31
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: 13 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 63005
Objects passed selection criteria: 62736
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 4
Average stars detected per image: 35924.8
Average stars matched: 34400.5 (95.7571 %)
Memory usage VmPeak: 163264 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 8 15:05:08 CDT 2026
VaST build number 1.0rc89-141-gc31ee76a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 10 06:59:04 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 --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
SExtractor catalog cache: saved Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat to cache
SExtractor catalog cache: saved Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.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/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.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: 2461231.84769322
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_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits exists and is non-empty
Saving wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits to local_wcs_cache/
'wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits' -> 'local_wcs_cache/wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits'
wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits exists and is non-empty
Saving wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits to local_wcs_cache/
'wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits' -> 'local_wcs_cache/wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits'
wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits exists and is non-empty
Saving wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits to local_wcs_cache/
'wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits' -> 'local_wcs_cache/wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits'
wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits exists and is non-empty
Saving wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits to local_wcs_cache/
'wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits' -> 'local_wcs_cache/wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits (1st reference image)
verification OK: wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:59:58.313 +29:59:11.22 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_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits (1st new image)
verification OK: wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
Image size: 941.5'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:00:11.899 +29:59:53.17 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:59:58.313 +29:59:11.22
Second-epoch image center 01:00:11.899 +29:59:53.17
Angular distance between the image centers 0.0504 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits (2nd new image)
verification OK: wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
Image size: 941.4'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:00:09.083 +30:00:11.68 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:59:58.313 +29:59:11.22
Second-epoch image center 01:00:09.083 +30:00:11.68
Angular distance between the image centers 0.0423 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 01:00:11.899 +29:59:53.17
Second-epoch second image center 01:00:09.083 +30:00:11.68
Angular distance between the image centers 0.01139 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/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits &> /tmp/tmp.qm57AQ7pUQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits &> /tmp/tmp.VsKuAdfhxL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits &> /tmp/tmp.KcZyjPOvQQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits &> /tmp/tmp.SlabKB4ZFe
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.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_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits and wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.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_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits and wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.wcscat
Found non-empty wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits and wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.wcscat
The reference image (wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits) and catalog (wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.wcscat) found
'wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.wcscat' -> 'wcsmag.cat'
Read 12201 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 5.5660 to 24.6535 deg, Dec +24.3268 to +35.2840 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 5.5660 to 24.6535 deg, Dec 24.3268 to 35.2840 deg
Loaded 8109 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): 6156 out of 6514 total matches.
Matched with Tycho-2 6514 out of 12201 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.935700
a=0.000000 b=1.000000 c=22.935700
From vast_summary.log: estimated ref. image limiting mag.: -7.55
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.39
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.39
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 12201 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 5.5660 to 24.6535 deg, Dec +24.3268 to +35.2840 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 5.5660 to 24.6535 deg, Dec 24.3268 to 35.2840 deg
Loaded 8109 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): 6156 out of 6514 total matches.
Matched with Tycho-2 6514 out of 12201 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits:
Forced-photometry filter: calibrated wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits -> calib.txt_param_ref_wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits (aperture=6.1)
Read 11480 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 5.6208 to 24.7112 deg, Dec +24.3682 to +35.3105 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 5.6208 to 24.7112 deg, Dec 24.3682 to 35.3105 deg
Loaded 8115 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): 6080 out of 6460 total matches.
Matched with Tycho-2 6460 out of 11480 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits:
Forced-photometry filter: calibrated wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits -> calib.txt_param_ref_wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
2.0 pix Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
2.6 pix fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
2.6 pix fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
2.1 pix wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
2.0 pix wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
Limiting magnitude estimates:
15.4 mag. Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
15.4 mag. Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
11.1 mag. fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
11.6 mag. fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
All-image limiting magnitude estimate: 11.1 (SNR ) 9.0 (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.qm57AQ7pUQ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits' -> 'wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
WCS_IMAGE_NAME=wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
WCS-calibrated image found: wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
Checking if the catalog wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.wcscat corresponding to the image wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits alredy exist and is non-empty...
Catalog wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.wcscat corresponding to the image wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
WCS catalog name: wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.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=849, bad_region=1, passed=12201
Got 12201 stars (including 11338 good ones) from the SExtractor catalog wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.wcscat
util/solve_plate_with_UCAC5 got 12201 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 12028 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 12027 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 12027 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits N_match=953 sigma_overall_arcsec=0.318 sigma_q1_arcsec=0.367 sigma_q2_arcsec=0.329 sigma_q3_arcsec=0.300 sigma_q4_arcsec=0.250 n_q1=246 n_q2=260 n_q3=190 n_q4=257 worst_quadrant_to_overall_ratio=1.155
The image catalog is written to wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits -region wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.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.VsKuAdfhxL (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits' -> 'wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
WCS_IMAGE_NAME=wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
WCS-calibrated image found: wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
Checking if the catalog wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.wcscat corresponding to the image wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits alredy exist and is non-empty...
Catalog wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.wcscat corresponding to the image wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
WCS catalog name: wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.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=846, bad_region=0, passed=11480
Got 11480 stars (including 10619 good ones) from the SExtractor catalog wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.wcscat
util/solve_plate_with_UCAC5 got 11480 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
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 11339 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
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 11337 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 11337 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits N_match=954 sigma_overall_arcsec=0.372 sigma_q1_arcsec=0.470 sigma_q2_arcsec=0.379 sigma_q3_arcsec=0.364 sigma_q4_arcsec=0.305 n_q1=240 n_q2=259 n_q3=196 n_q4=259 worst_quadrant_to_overall_ratio=1.264
The image catalog is written to wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits -region wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.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.KcZyjPOvQQ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
WCS_IMAGE_NAME=wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
WCS-calibrated image found: wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
Checking if the catalog wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat corresponding to the image wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat corresponding to the image wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
WCS catalog name: wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.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=11, bad_region=0, passed=395
Got 395 stars (including 384 good ones) from the SExtractor catalog wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat
util/solve_plate_with_UCAC5 got 395 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
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 629 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 353 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 352 matched stars entering correct_measured_positions(), 252 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 352 matched stars entering correct_measured_positions(), 282 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 629 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 353 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 352 matched stars entering correct_measured_positions(), 282 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Accuracy estimation diagnostic: 352 matched stars entering correct_measured_positions(), 282 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 352 stars left (next iteration limit 387)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits N_match=352 sigma_overall_arcsec=0.680 sigma_q1_arcsec=0.597 sigma_q2_arcsec=0.806 sigma_q3_arcsec=0.630 sigma_q4_arcsec=0.609 n_q1=98 n_q2=51 n_q3=112 n_q4=91 worst_quadrant_to_overall_ratio=1.185
The image catalog is written to wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits -region wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.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.SlabKB4ZFe (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
WCS_IMAGE_NAME=wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
WCS-calibrated image found: wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
Checking if the catalog wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat corresponding to the image wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat corresponding to the image wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
WCS catalog name: wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.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=22, bad_region=0, passed=473
Got 473 stars (including 450 good ones) from the SExtractor catalog wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat
util/solve_plate_with_UCAC5 got 473 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.6 to 35.4)
Done reading UCAC5 zone files...
Matched 413 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 412 matched stars entering correct_measured_positions(), 335 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 412 matched stars entering correct_measured_positions(), 380 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.6 to 35.4)
Done reading UCAC5 zone files...
Matched 413 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 411 matched stars entering correct_measured_positions(), 377 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 411 matched stars entering correct_measured_positions(), 377 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 411 stars left (next iteration limit 453)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits N_match=411 sigma_overall_arcsec=0.511 sigma_q1_arcsec=0.477 sigma_q2_arcsec=0.393 sigma_q3_arcsec=0.481 sigma_q4_arcsec=0.606 n_q1=129 n_q2=67 n_q3=165 n_q4=50 worst_quadrant_to_overall_ratio=1.186
The image catalog is written to wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits -region wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.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=Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits sigma_overall=0.318 worst_q_ratio=1.155
ref2=Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits sigma_overall=0.372 worst_q_ratio=1.264
new1=fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits sigma_overall=0.680 worst_q_ratio=1.185
new2=fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits sigma_overall=0.511 worst_q_ratio=1.186
reference average sigma_overall=0.345 worst_q_ratio=1.2095
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181_astrometric_residuals.png (953 matched stars from wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096_astrometric_residuals.png (954 matched stars from wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312_astrometric_residuals.png (352 matched stars from wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.63 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313_astrometric_residuals.png (411 matched stars from wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.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_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits'
Saving fully-calibrated image wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits'
Preparing the HTML report for the field Psc-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Psc-01-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 --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
SExtractor catalog cache: saved Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat to cache
SExtractor catalog cache: saved Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
Creating symlink local_wcs_cache/wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.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_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits exists and is non-empty
wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits exists and is non-empty
wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits exists and is non-empty
wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits (1st reference image)
verification OK: wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:59:58.313 +29:59:11.22 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_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits (1st new image)
verification OK: wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
Image size: 941.5'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:00:11.899 +29:59:53.17 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:59:58.313 +29:59:11.22
Second-epoch image center 01:00:11.899 +29:59:53.17
Angular distance between the image centers 0.0504 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits (2nd new image)
verification OK: wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
Image size: 941.4'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:00:09.083 +30:00:11.68 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:59:58.313 +29:59:11.22
Second-epoch image center 01:00:09.083 +30:00:11.68
Angular distance between the image centers 0.0423 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 01:00:11.899 +29:59:53.17
Second-epoch second image center 01:00:09.083 +30:00:11.68
Angular distance between the image centers 0.01139 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/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits &> /tmp/tmp.BDhpNN7eBO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits &> /tmp/tmp.MrN9WyX9Qn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits &> /tmp/tmp.QWaH8AOWIt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits &> /tmp/tmp.eDRn83UJH4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.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_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits and wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.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_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits and wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.wcscat
Found non-empty wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits and wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.wcscat
The reference image (wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits) and catalog (wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.wcscat) found
'wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.wcscat' -> 'wcsmag.cat'
Read 67418 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 5.5660 to 24.6789 deg, Dec +24.2962 to +35.2922 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 5.5660 to 24.6789 deg, Dec 24.2962 to 35.2922 deg
Loaded 8148 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): 5658 out of 6593 total matches.
Matched with Tycho-2 6593 out of 67418 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.833800
a=0.000000 b=1.000000 c=22.833800
From vast_summary.log: estimated ref. image limiting mag.: -7.31
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.52
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.52
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 67418 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 5.5660 to 24.6789 deg, Dec +24.2962 to +35.2922 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 5.5660 to 24.6789 deg, Dec 24.2962 to 35.2922 deg
Loaded 8148 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): 5658 out of 6593 total matches.
Matched with Tycho-2 6593 out of 67418 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits:
Forced-photometry filter: calibrated wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits -> calib.txt_param_ref_wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits (aperture=4.9)
Read 69317 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 5.5774 to 24.7112 deg, Dec +24.3307 to +35.3186 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 5.5774 to 24.7112 deg, Dec 24.3307 to 35.3186 deg
Loaded 8155 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): 5653 out of 6601 total matches.
Matched with Tycho-2 6601 out of 69317 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits:
Forced-photometry filter: calibrated wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits -> calib.txt_param_ref_wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 21 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
1.9 pix Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
2.5 pix fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
2.5 pix fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
2.0 pix wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
1.9 pix wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
Limiting magnitude estimates:
15.5 mag. Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
15.5 mag. Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
11.6 mag. fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
11.9 mag. fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
All-image limiting magnitude estimate: 11.6 (SNR ) 11.0 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.BDhpNN7eBO (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits' -> 'wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
WCS_IMAGE_NAME=wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
WCS-calibrated image found: wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
Checking if the catalog wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.wcscat corresponding to the image wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits alredy exist and is non-empty...
Catalog wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.wcscat corresponding to the image wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
WCS catalog name: wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.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=16, blended=4197, bad_region=9, passed=67402
Got 67402 stars (including 63070 good ones) from the SExtractor catalog wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.wcscat
util/solve_plate_with_UCAC5 got 67402 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 66531 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 66532 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 66532 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits N_match=959 sigma_overall_arcsec=0.298 sigma_q1_arcsec=0.343 sigma_q2_arcsec=0.310 sigma_q3_arcsec=0.258 sigma_q4_arcsec=0.242 n_q1=249 n_q2=257 n_q3=201 n_q4=252 worst_quadrant_to_overall_ratio=1.150
The image catalog is written to wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits -region wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.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.MrN9WyX9Qn (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits' -> 'wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
WCS_IMAGE_NAME=wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
WCS-calibrated image found: wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
Checking if the catalog wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.wcscat corresponding to the image wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits alredy exist and is non-empty...
Catalog wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.wcscat corresponding to the image wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
WCS catalog name: wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.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=36, blended=4253, bad_region=7, passed=69281
Got 69281 stars (including 64921 good ones) from the SExtractor catalog wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.wcscat
util/solve_plate_with_UCAC5 got 69281 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
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 68370 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
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 68366 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 68366 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits N_match=959 sigma_overall_arcsec=0.358 sigma_q1_arcsec=0.421 sigma_q2_arcsec=0.381 sigma_q3_arcsec=0.339 sigma_q4_arcsec=0.306 n_q1=241 n_q2=256 n_q3=205 n_q4=257 worst_quadrant_to_overall_ratio=1.174
The image catalog is written to wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits -region wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.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.QWaH8AOWIt (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
WCS_IMAGE_NAME=wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
WCS-calibrated image found: wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
Checking if the catalog wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat corresponding to the image wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat corresponding to the image wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
WCS catalog name: wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=53, bad_region=6, passed=3772
Got 3772 stars (including 3702 good ones) from the SExtractor catalog wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat
util/solve_plate_with_UCAC5 got 3772 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
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 3656 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 3655 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 3655 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits N_match=935 sigma_overall_arcsec=0.565 sigma_q1_arcsec=0.570 sigma_q2_arcsec=0.708 sigma_q3_arcsec=0.525 sigma_q4_arcsec=0.547 n_q1=250 n_q2=147 n_q3=310 n_q4=228 worst_quadrant_to_overall_ratio=1.254
The image catalog is written to wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits -region wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.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.eDRn83UJH4 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
WCS_IMAGE_NAME=wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
WCS-calibrated image found: wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
Checking if the catalog wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat corresponding to the image wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat corresponding to the image wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
WCS catalog name: wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.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=47, bad_region=4, passed=4108
Got 4108 stars (including 4048 good ones) from the SExtractor catalog wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat
util/solve_plate_with_UCAC5 got 4108 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 629 (Dec 24.4 to 35.4)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 899 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 3918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 629 (Dec 24.4 to 35.4)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 3921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 3921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits N_match=932 sigma_overall_arcsec=0.480 sigma_q1_arcsec=0.522 sigma_q2_arcsec=0.448 sigma_q3_arcsec=0.431 sigma_q4_arcsec=0.651 n_q1=247 n_q2=147 n_q3=418 n_q4=120 worst_quadrant_to_overall_ratio=1.355
The image catalog is written to wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits -region wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.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_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-20-30_20.00sec_-0.00C_LIGHTs_0312.fits
Saving fully-calibrated image wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-01-Q1b1x1_033157_TTUQ1b1x1_1211655_homj6G8g/wcs_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313.fits
Preparing the HTML report for the field Psc-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:26:14.45 +34:21:12.1: 11.69 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:35:36.70 +34:51:05.1: 11.86 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:25:12.88 +27:43:51.8: 11.60 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:36:16.94 +34:44:34.7: 12.13 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:36:09.04 +29:07:33.1: 12.30 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:25:41.96 +34:07:00.7: 12.27 +/- 0.02 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:25:41.97 +27:46:14.9: 12.07 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:26:17.80 +34:20:14.6: 11.56 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:36:10.48 +29:23:37.7: 12.16 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:53:51.65 +34:31:20.0: 12.11 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:26:14.45 +34:21:12.1: 11.72 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:25:41.96 +34:07:00.7: 12.29 +/- 0.02 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:25:41.97 +27:46:14.9: 12.09 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:35:36.70 +34:51:05.1: 11.89 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:26:17.80 +34:20:14.6: 11.60 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:36:16.94 +34:44:34.7: 12.16 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:36:10.48 +29:23:37.7: 12.23 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:53:51.65 +34:31:20.0: 12.14 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:36:09.04 +29:07:33.1: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.70 +/- 0.01
Forced photometry reference-image weighted average: 12.28 +/- 0.01
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:25:12.88 +27:43:51.8: 11.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.87 +/- 0.01
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Forced photometry reference-image weighted average: 11.58 +/- 0.01
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Forced photometry filter KEPT candidate at 00:26:14.45 +34:21:12.1: ref_mag=11.70 +/- 0.01 new_mean_mag=10.6774 delta=1.03 (need > 0.90)
Forced photometry filter KEPT candidate at 00:25:41.96 +34:07:00.7: ref_mag=12.28 +/- 0.01 new_mean_mag=11.1362 delta=1.14 (need > 0.90)
Forced photometry filter KEPT candidate at 00:36:16.94 +34:44:34.7: ref_mag=12.14 +/- 0.01 new_mean_mag=11.1629 delta=0.98 (need > 0.90)
Forced photometry filter KEPT candidate at 00:26:17.80 +34:20:14.6: ref_mag=11.58 +/- 0.01 new_mean_mag=10.5958 delta=0.98 (need > 0.90)
Forced photometry filter KEPT candidate at 00:35:36.70 +34:51:05.1: ref_mag=11.87 +/- 0.01 new_mean_mag=10.7800 delta=1.09 (need > 0.90)
Forced photometry filter KEPT candidate at 00:25:41.97 +27:46:14.9: ref_mag=12.08 +/- 0.01 new_mean_mag=11.0095 delta=1.07 (need > 0.90)
Forced photometry filter KEPT candidate at 00:36:10.48 +29:23:37.7: ref_mag=12.19 +/- 0.01 new_mean_mag=11.1069 delta=1.09 (need > 0.90)
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Forced photometry filter KEPT candidate at 00:53:51.65 +34:31:20.0: ref_mag=12.13 +/- 0.01 new_mean_mag=11.1579 delta=0.97 (need > 0.90)
Forced photometry reference-image weighted average: 11.62 +/- 0.01
Forced photometry filter KEPT candidate at 00:36:09.04 +29:07:33.1: ref_mag=12.31 +/- 0.01 new_mean_mag=11.2910 delta=1.02 (need > 0.90)
Forced photometry filter KEPT candidate at 00:25:12.88 +27:43:51.8: ref_mag=11.62 +/- 0.01 new_mean_mag=10.6441 delta=0.98 (need > 0.90)
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:25:55.41 +34:13:09.0: 11.57 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:35:47.38 +34:49:12.8: 11.50 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:25:55.41 +34:13:09.0: 11.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.56 +/- 0.01
Forced photometry filter KEPT candidate at 00:25:55.41 +34:13:09.0: ref_mag=11.56 +/- 0.01 new_mean_mag=10.5481 delta=1.02 (need > 0.90)
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:35:47.38 +34:49:12.8: 11.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.51 +/- 0.00
Forced photometry filter KEPT candidate at 00:35:47.38 +34:49:12.8: ref_mag=11.51 +/- 0.00 new_mean_mag=10.5319 delta=0.98 (need > 0.90)
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:33:48.29 +31:17:59.0: 11.47 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:33:48.29 +31:17:59.0: 11.48 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.48 +/- 0.00
Forced photometry filter KEPT candidate at 00:33:48.29 +31:17:59.0: ref_mag=11.48 +/- 0.00 new_mean_mag=10.5004 delta=0.98 (need > 0.90)
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:35:43.32 +34:49:15.6: 11.45 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:35:22.09 +34:58:08.6: 12.01 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:36:31.42 +29:21:37.4: 12.01 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:36:13.65 +34:54:04.5: 11.91 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:35:43.32 +34:49:15.6: 11.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.47 +/- 0.00
Forced photometry filter KEPT candidate at 00:35:43.32 +34:49:15.6: ref_mag=11.47 +/- 0.00 new_mean_mag=10.4952 delta=0.98 (need > 0.90)
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:35:22.09 +34:58:08.6: 12.02 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.01
Forced photometry filter KEPT candidate at 00:35:22.09 +34:58:08.6: ref_mag=12.02 +/- 0.01 new_mean_mag=10.9412 delta=1.08 (need > 0.90)
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:36:31.42 +29:21:37.4: 12.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.04 +/- 0.01
Forced photometry filter KEPT candidate at 00:36:31.42 +29:21:37.4: ref_mag=12.04 +/- 0.01 new_mean_mag=10.9359 delta=1.11 (need > 0.90)
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:36:13.65 +34:54:04.5: 11.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.93 +/- 0.01
Forced photometry filter KEPT candidate at 00:36:13.65 +34:54:04.5: ref_mag=11.93 +/- 0.01 new_mean_mag=10.9839 delta=0.95 (need > 0.90)
Forced photometry on wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:25:34.61 +34:13:04.3: 11.90 +/- 0.01 detection
Forced photometry on wcs_Psc-01-Q1b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:25:34.61 +34:13:04.3: 11.93 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Forced photometry filter KEPT candidate at 00:25:34.61 +34:13:04.3: ref_mag=11.92 +/- 0.01 new_mean_mag=10.6371 delta=1.28 (need > 0.90)
Adding exclusion_list_local.txt__out01810.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02373.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02696.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02857.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02938.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03561.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05516.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05631.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05736.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06370.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28315.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41390.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41585.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43097.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61781.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62155.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 33s
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: 11s
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Considering the candidate 61781_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 61781_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 05736_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 05736_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 02696_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 02696_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 43097_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 43097_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 07208_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 07208_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 62155_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 62155_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 05631_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 05631_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 41390_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 41390_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 03561_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 03561_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 05516_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 05516_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 06512_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 06512_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 02857_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 02857_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 28315_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 28315_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 02938_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 02938_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 01810_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 01810_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 41585_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 41585_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 02373_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 02373_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 30205_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
The candidate 30205_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313 did not pass the final checks
**** FOUND 00:39:20.05 +30:51:37.9 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 41096_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
The candidate 41096_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313 did not pass the final checks
**** FOUND 00:38:32.99 +29:18:35.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 06370_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 06370_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 37947_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313
The candidate 37947_fd_Psc-01-Q1b1x1_2026-07-10_03-23-52_20.00sec_-0.00C_LIGHTs_0313 did not pass the final checks
