This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL
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 10.3493 2461231.8493 12.26 01:40:38.50 +09:56:13.9
142.43749 -51.06158 galactic Psc Second-epoch detections are separated by 0.9" and 4.9 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 | target | 01:40:38.50 +09:56:13.9 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.581+/-0.033 (K)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:40:38.50 +09:56:13.9: 13.38 +/- 0.03 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:40:38.50 +09:56:13.9: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8493,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3493 12.26CV 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 10.3493 2461231.8493 12.20 01:53:03.57 +16:33:15.8
143.60145 -43.83032 galactic Ari Second-epoch detections are separated by 0.5" and 4.7 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 | target | 01:53:03.57 +16:33:15.8 (user input) | T | P | (position from user input) J-Ks=0.417+/-0.029 (G)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:53:03.57 +16:33:15.8: 13.22 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:53:03.57 +16:33:15.8: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3493* 01 53 03.57 +16 33 15.8 12.2 U Ari 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
target,2461231.8493,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3493 12.20CV 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 10.3493 2461231.8493 12.33 01:54:40.28 +17:56:29.4
143.47621 -42.39372 galactic Ari Second-epoch detections are separated by 3.2" and 5.3 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 91926013965610624 | 01:54:40.26 +17:56:56.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.353+/-0.031 (G)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:54:40.28 +17:56:29.4: 13.46 +/- 0.03 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:54:40.28 +17:56:29.4: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3493* 01 54 40.28 +17 56 29.4 12.3 U Ari 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 91926013965610624,2461231.8493,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 91926013965610624 20260710.3493 12.33CV 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 10.3493 2461231.8493 11.96 01:53:26.30 +17:58:06.3
143.08869 -42.46367 galactic Ari Second-epoch detections are separated by 0.1" and 4.8 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 | target | 01:53:26.30 +17:58:06.3 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.366+/-0.028 (G)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:53:26.30 +17:58:06.3: 12.85 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:53:26.30 +17:58:06.3: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 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 10.3493* 01 53 26.30 +17 58 06.3 12.0 U Ari 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
target,2461231.8493,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3493 11.96CV 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 10.3493 2461231.8493 12.01 01:53:00.35 +17:25:30.6
143.19465 -43.01110 galactic Ari Second-epoch detections are separated by 0.8" and 4.9 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 | target | 01:53:00.35 +17:25:30.6 (user input) | T | P | (position from user input) J-Ks=0.376+/-0.028 (G)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:53:00.35 +17:25:30.6: 12.88 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:53:00.35 +17:25:30.6: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 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 10.3493* 01 53 00.35 +17 25 30.6 12.0 U Ari 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
target,2461231.8493,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3493 12.01CV 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 10.3493 2461231.8493 11.96 01:38:14.13 +10:01:42.7
141.49299 -51.14889 galactic Psc Second-epoch detections are separated by 0.9" and 4.9 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 | target | 01:38:14.13 +10:01:42.7 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.350+/-0.037 (G)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:38:14.13 +10:01:42.7: 12.90 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:38:14.13 +10:01:42.7: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8493,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3493 11.96CV 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 10.3493 2461231.8493 12.00 01:52:38.19 +17:25:45.7
143.07872 -43.03551 galactic Ari Second-epoch detections are separated by 0.3" and 4.8 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 | target | 01:52:38.19 +17:25:45.7 (user input) | T | P | (position from user input) J-Ks=0.377+/-0.029 (G)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:52:38.19 +17:25:45.7: 12.98 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:52:38.19 +17:25:45.7: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 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 10.3493* 01 52 38.19 +17 25 45.7 12.0 U Ari 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
target,2461231.8493,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3493 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3493 2461231.8493 12.07 01:53:07.24 +17:28:29.1
143.20817 -42.95532 galactic Ari Second-epoch detections are separated by 0.8" and 4.9 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 | target | 01:53:07.24 +17:28:29.1 (user input) | T | P | (position from user input) J-Ks=0.302+/-0.031 (F)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:53:07.24 +17:28:29.1: 13.00 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:53:07.24 +17:28:29.1: 13.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 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 10.3493* 01 53 07.24 +17 28 29.1 12.1 U Ari 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
target,2461231.8493,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3493 12.07CV 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 10.3493 2461231.8493 11.79 01:52:20.08 +17:12:35.0
143.08189 -43.26665 galactic Ari Second-epoch detections are separated by 1.6" and 5.0 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 | target | 01:52:20.08 +17:12:35.0 (user input) | T | P | (position from user input) J-Ks=0.569+/-0.027 (K)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:52:20.08 +17:12:35.0: 12.86 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:52:20.08 +17:12:35.0: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 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 10.3493* 01 52 20.08 +17 12 35.0 11.8 U Ari 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
target,2461231.8493,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3493 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3493 2461231.8493 11.96 01:52:51.74 +17:20:15.7
143.18896 -43.10494 galactic Ari Second-epoch detections are separated by 2.1" and 4.5 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 | target | 01:52:51.74 +17:20:15.7 (user input) | T | P | (position from user input) J-Ks=0.618+/-0.027 (K)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:52:51.74 +17:20:15.7: 12.85 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:52:51.74 +17:20:15.7: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 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 10.3493* 01 52 51.74 +17 20 15.7 12.0 U Ari 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
target,2461231.8493,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3493 11.96CV 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 10.3493 2461231.8493 11.59 01:38:23.04 +09:47:53.0
141.65528 -51.35898 galactic Psc Second-epoch detections are separated by 1.2" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.2501 Lohja -559 -183 588 17.2 -0 -0
ATTENTION: measured mag 11.59 is 5.6 mag brighter than the predicted asteroid brightness 17.2 - the transient may be an unrelated new object!
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:38:23.04 +09:47:53.0: 12.56 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:38:23.04 +09:47:53.0: 12.48 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461231.8493,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260710.3493 11.59CV 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 10.3493 2461231.8493 12.20 01:50:46.84 +17:01:56.7
142.67481 -43.55272 galactic Ari Second-epoch detections are separated by 3.9" and 4.7 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 | target | 01:50:46.84 +17:01:56.7 (user input) | T | P | (position from user input) J-Ks=0.613+/-0.027 (K)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:50:46.84 +17:01:56.7: 13.17 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:50:46.84 +17:01:56.7: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3493* 01 50 46.84 +17 01 56.7 12.2 U Ari 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
target,2461231.8493,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3493 12.20CV 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 10.3493 2461231.8493 12.29 01:53:43.26 +18:00:34.9
143.15681 -42.40290 galactic Ari Second-epoch detections are separated by 2.0" and 4.5 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 | target | 01:53:43.26 +18:00:34.9 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.701+/-0.028 (K)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:53:43.26 +18:00:34.9: 13.35 +/- 0.03 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:53:43.26 +18:00:34.9: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3493* 01 53 43.26 +18 00 34.9 12.3 U Ari 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
target,2461231.8493,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3493 12.29CV 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 10.3493 2461231.8493 12.17 01:42:41.08 +12:26:36.9
142.01396 -48.52026 galactic Psc Second-epoch detections are separated by 1.8" and 4.9 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 | target | 01:42:41.08 +12:26:36.9 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.686+/-0.029 (K)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:42:41.08 +12:26:36.9: 13.13 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:42:41.08 +12:26:36.9: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8493,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3493 12.17CV 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 10.3493 2461231.8493 12.12 01:54:19.91 +17:55:44.4
143.37842 -42.43198 galactic Ari Second-epoch detections are separated by 1.7" and 4.9 pix
The object was found in VSX 0" Gaia DR3 91925361130473984
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.970 G 13.000 G F
The object was not found in astcheck.
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:54:19.91 +17:55:44.4: 13.13 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:54:19.91 +17:55:44.4: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3493* 01 54 19.91 +17 55 44.4 12.1 U Ari 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 91925361130473984,2461231.8493,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 91925361130473984 20260710.3493 12.12CV 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 10.3493 2461231.8493 11.78 01:37:38.76 +09:43:20.3
141.41104 -51.48390 galactic Psc Second-epoch detections are separated by 1.7" and 4.9 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 | target | 01:37:38.76 +09:43:20.3 (user input) | T | P | (position from user input) J-Ks=0.351+/-0.035 (G)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:37:38.76 +09:43:20.3: 12.75 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:37:38.76 +09:43:20.3: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8493,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3493 11.78CV 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 10.3493 2461231.8493 12.18 01:52:24.63 +17:07:12.8
143.14498 -43.34558 galactic Ari Second-epoch detections are separated by 0.3" and 4.8 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 | target | 01:52:24.63 +17:07:12.8 (user input) | T | P | (position from user input) J-Ks=0.450+/-0.036 (G)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:52:24.63 +17:07:12.8: 13.11 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:52:24.63 +17:07:12.8: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3493* 01 52 24.63 +17 07 12.8 12.2 U Ari 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
target,2461231.8493,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3493 12.18CV 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 10.3493 2461231.8493 11.74 01:39:59.21 +11:09:59.4
141.62339 -49.93509 galactic Psc Second-epoch detections are separated by 1.6" and 4.8 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 2573737436773353600 | 01:39:59.18 +11:09:59.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.403+/-0.031 (G)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:39:59.21 +11:09:59.4: 12.71 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:39:59.21 +11:09:59.4: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 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!
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 2573737436773353600,2461231.8493,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2573737436773353600 20260710.3493 11.74CV 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: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
First image: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Last image: 2461231.84960374 10.07.2026 08:23:15.763 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.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: 6 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): 5117
Objects passed selection criteria: 5074
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 3027
Average stars matched: 2979.75 (98.439 %)
Memory usage VmPeak: 111936 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 05:53:42 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
First image: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Last image: 2461231.84960374 10.07.2026 08:23:15.763 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 30
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.26
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 20 seconds
Number of parallel threads: 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): 28497
Objects passed selection criteria: 28398
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 18019.5
Average stars matched: 17574.8 (97.5318 %)
Memory usage VmPeak: 134608 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 05:56:27 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
SExtractor catalog cache: saved Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.cat to cache
SExtractor catalog cache: saved Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.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-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.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: 2461231.84905458
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-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits exists and is non-empty
Saving wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits to local_wcs_cache/
'wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits' -> 'local_wcs_cache/wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits'
wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits exists and is non-empty
Saving wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits to local_wcs_cache/
'wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits' -> 'local_wcs_cache/wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits'
wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits exists and is non-empty
Saving wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits to local_wcs_cache/
'wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits' -> 'local_wcs_cache/wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits'
wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits exists and is non-empty
Saving wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits to local_wcs_cache/
'wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits' -> 'local_wcs_cache/wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (1st reference image)
verification OK: wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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: 01:46:39.828 +14:00:12.80 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-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits (1st new image)
verification OK: wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits
Image size: 939.0'x624.3' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:46:38.601 +13:59:58.45 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:46:39.828 +14:00:12.80
Second-epoch image center 01:46:38.601 +13:59:58.45
Angular distance between the image centers 0.0064 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits (2nd new image)
verification OK: wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
Image size: 938.9'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:46:37.955 +13:59:31.92 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:46:39.828 +14:00:12.80
Second-epoch image center 01:46:37.955 +13:59:31.92
Angular distance between the image centers 0.0136 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 01:46:38.601 +13:59:58.45
Second-epoch second image center 01:46:37.955 +13:59:31.92
Angular distance between the image centers 0.00782 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-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits &> /tmp/tmp.tcO4rEfcaP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits &> /tmp/tmp.K68OR3lSCq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits &> /tmp/tmp.VsrU5GuRNC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits &> /tmp/tmp.gh5Alhnlor
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
Found non-empty wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
The reference image (wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits) and catalog (wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat) found
'wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat' -> 'wcsmag.cat'
Read 7679 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.3971 to 34.9280 deg, Dec +8.6500 to +19.2744 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 18.3971 to 34.9280 deg, Dec 8.6500 to 19.2744 deg
Loaded 4730 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): 3854 out of 4067 total matches.
Matched with Tycho-2 4067 out of 7679 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.943700
a=0.000000 b=1.000000 c=22.943700
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 7679 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.3971 to 34.9280 deg, Dec +8.6500 to +19.2744 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 18.3971 to 34.9280 deg, Dec 8.6500 to 19.2744 deg
Loaded 4730 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): 3854 out of 4067 total matches.
Matched with Tycho-2 4067 out of 7679 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits:
Forced-photometry filter: calibrated wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits -> calib.txt_param_ref_wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (aperture=5.9)
Read 6663 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.4568 to 34.9561 deg, Dec +8.6500 to +19.2743 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 18.4568 to 34.9561 deg, Dec 8.6500 to 19.2743 deg
Loaded 4716 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): 3860 out of 4017 total matches.
Matched with Tycho-2 4017 out of 6663 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits:
Forced-photometry filter: calibrated wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits -> calib.txt_param_ref_wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits (aperture=6.2)
____ 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:
2.0 pix Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
2.2 pix Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
2.3 pix fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits
2.3 pix fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
2.0 pix wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
2.2 pix wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
Limiting magnitude estimates:
15.4 mag. Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
15.1 mag. Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
11.9 mag. fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits
12.0 mag. fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
All-image limiting magnitude estimate: 11.9 (SNR ) 9.8 (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.tcO4rEfcaP (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits is already a symlink and we do not allow symlinks on symlinks
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-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits' -> 'wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS-calibrated image found: wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Checking if the catalog wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS catalog name: wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=549, bad_region=1800, passed=7679
Got 7679 stars (including 5466 good ones) from the SExtractor catalog wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
util/solve_plate_with_UCAC5 got 7679 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 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 5975 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 5976 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 5976 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits N_match=972 sigma_overall_arcsec=0.290 sigma_q1_arcsec=0.342 sigma_q2_arcsec=0.242 sigma_q3_arcsec=0.250 sigma_q4_arcsec=0.244 n_q1=292 n_q2=189 n_q3=313 n_q4=178 worst_quadrant_to_overall_ratio=1.181
The image catalog is written to wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits -region wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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.K68OR3lSCq (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits is already a symlink and we do not allow symlinks on symlinks
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-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.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-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits' -> 'wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
WCS-calibrated image found: wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
Checking if the catalog wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat corresponding to the image wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat corresponding to the image wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
WCS catalog name: wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=444, bad_region=1535, passed=6663
Got 6663 stars (including 4786 good ones) from the SExtractor catalog wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat
util/solve_plate_with_UCAC5 got 6663 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 5238 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 5237 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 5237 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits N_match=974 sigma_overall_arcsec=0.300 sigma_q1_arcsec=0.344 sigma_q2_arcsec=0.289 sigma_q3_arcsec=0.272 sigma_q4_arcsec=0.269 n_q1=300 n_q2=191 n_q3=314 n_q4=169 worst_quadrant_to_overall_ratio=1.145
The image catalog is written to wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits -region wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.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.VsrU5GuRNC (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-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.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-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits
Checking if the catalog wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.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-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits
WCS catalog name: wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=48, bad_region=276, passed=868
Got 868 stars (including 553 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits.wcscat
util/solve_plate_with_UCAC5 got 868 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 528 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 527 matched stars entering correct_measured_positions(), 485 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 527 matched stars entering correct_measured_positions(), 573 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 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 528 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 527 matched stars entering correct_measured_positions(), 577 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 527 matched stars entering correct_measured_positions(), 577 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 527 stars left (next iteration limit 579)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits N_match=527 sigma_overall_arcsec=0.468 sigma_q1_arcsec=0.484 sigma_q2_arcsec=0.422 sigma_q3_arcsec=0.699 sigma_q4_arcsec=0.413 n_q1=183 n_q2=150 n_q3=72 n_q4=122 worst_quadrant_to_overall_ratio=1.493
The image catalog is written to wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits -region wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.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.gh5Alhnlor (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-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.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-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
Checking if the catalog wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.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-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
WCS catalog name: wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=50, bad_region=277, passed=854
Got 854 stars (including 540 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits.wcscat
util/solve_plate_with_UCAC5 got 854 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 511 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 510 matched stars entering correct_measured_positions(), 471 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 510 matched stars entering correct_measured_positions(), 554 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 511 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 510 matched stars entering correct_measured_positions(), 556 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 510 matched stars entering correct_measured_positions(), 556 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 510 stars left (next iteration limit 561)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits N_match=510 sigma_overall_arcsec=0.459 sigma_q1_arcsec=0.410 sigma_q2_arcsec=0.467 sigma_q3_arcsec=0.551 sigma_q4_arcsec=0.467 n_q1=164 n_q2=150 n_q3=73 n_q4=123 worst_quadrant_to_overall_ratio=1.201
The image catalog is written to wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits -region wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.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-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits sigma_overall=0.290 worst_q_ratio=1.181
ref2=Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits sigma_overall=0.300 worst_q_ratio=1.145
new1=fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits sigma_overall=0.468 worst_q_ratio=1.493
new2=fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits sigma_overall=0.459 worst_q_ratio=1.201
reference average sigma_overall=0.295 worst_q_ratio=1.163
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_astrometric_residuals.png (972 matched stars from wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_astrometric_residuals.png (974 matched stars from wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348_astrometric_residuals.png (527 matched stars from wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.42 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349_astrometric_residuals.png (510 matched stars from wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits'
Saving fully-calibrated image wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits'
Preparing the HTML report for the field Psc-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Psc-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
SExtractor catalog cache: saved Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.cat to cache
SExtractor catalog cache: saved Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.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-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Creating symlink local_wcs_cache/wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
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-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits exists and is non-empty
wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits exists and is non-empty
wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits exists and is non-empty
wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (1st reference image)
verification OK: wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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: 01:46:39.828 +14:00:12.80 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-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits (1st new image)
verification OK: wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits
Image size: 939.0'x624.3' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:46:38.601 +13:59:58.45 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:46:39.828 +14:00:12.80
Second-epoch image center 01:46:38.601 +13:59:58.45
Angular distance between the image centers 0.0064 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits (2nd new image)
verification OK: wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
Image size: 938.9'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:46:37.955 +13:59:31.92 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:46:39.828 +14:00:12.80
Second-epoch image center 01:46:37.955 +13:59:31.92
Angular distance between the image centers 0.0136 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 01:46:38.601 +13:59:58.45
Second-epoch second image center 01:46:37.955 +13:59:31.92
Angular distance between the image centers 0.00782 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-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits &> /tmp/tmp.TjFNJaJVL2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits &> /tmp/tmp.VHic3OzdzT
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits &> /tmp/tmp.XSifKywnUT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits &> /tmp/tmp.sIpphf4CYW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
Found non-empty wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
The reference image (wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits) and catalog (wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat) found
'wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat' -> 'wcsmag.cat'
Read 40639 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.3971 to 34.9782 deg, Dec +8.6329 to +19.2915 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 18.3971 to 34.9782 deg, Dec 8.6329 to 19.2915 deg
Loaded 4751 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): 3680 out of 4108 total matches.
Matched with Tycho-2 4108 out of 40639 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.837850
a=0.000000 b=1.000000 c=22.837850
From vast_summary.log: estimated ref. image limiting mag.: -7.26
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.58
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.58
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 40639 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.3971 to 34.9782 deg, Dec +8.6329 to +19.2915 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 18.3971 to 34.9782 deg, Dec 8.6329 to 19.2915 deg
Loaded 4751 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): 3680 out of 4108 total matches.
Matched with Tycho-2 4108 out of 40639 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits:
Forced-photometry filter: calibrated wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits -> calib.txt_param_ref_wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (aperture=4.7)
Read 35714 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.4024 to 35.0127 deg, Dec +8.5911 to +19.2852 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 18.4024 to 35.0127 deg, Dec 8.5911 to 19.2852 deg
Loaded 4781 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): 3749 out of 4114 total matches.
Matched with Tycho-2 4114 out of 35714 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits:
Forced-photometry filter: calibrated wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits -> calib.txt_param_ref_wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 20 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
2.1 pix Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
2.1 pix fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits
2.0 pix fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
2.0 pix wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
2.1 pix wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
Limiting magnitude estimates:
15.6 mag. Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
15.3 mag. Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
12.7 mag. fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits
12.5 mag. fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
All-image limiting magnitude estimate: 12.5 (SNR ) 12.4 (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.TjFNJaJVL2 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits is already a symlink and we do not allow symlinks on symlinks
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-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits' -> 'wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS-calibrated image found: wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Checking if the catalog wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS catalog name: wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=7, blended=1873, bad_region=7665, passed=40632
Got 40632 stars (including 31385 good ones) from the SExtractor catalog wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
util/solve_plate_with_UCAC5 got 40632 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 969 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 33589 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 33589 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 33589 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits N_match=972 sigma_overall_arcsec=0.280 sigma_q1_arcsec=0.344 sigma_q2_arcsec=0.229 sigma_q3_arcsec=0.240 sigma_q4_arcsec=0.218 n_q1=286 n_q2=203 n_q3=302 n_q4=181 worst_quadrant_to_overall_ratio=1.231
The image catalog is written to wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits -region wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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.VHic3OzdzT (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits is already a symlink and we do not allow symlinks on symlinks
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-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.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-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits' -> 'wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
WCS-calibrated image found: wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
Checking if the catalog wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat corresponding to the image wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat corresponding to the image wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
WCS catalog name: wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1568, bad_region=6870, passed=35703
Got 35703 stars (including 27553 good ones) from the SExtractor catalog wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat
util/solve_plate_with_UCAC5 got 35703 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29270 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29271 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29271 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits N_match=973 sigma_overall_arcsec=0.301 sigma_q1_arcsec=0.357 sigma_q2_arcsec=0.273 sigma_q3_arcsec=0.275 sigma_q4_arcsec=0.257 n_q1=292 n_q2=199 n_q3=306 n_q4=176 worst_quadrant_to_overall_ratio=1.185
The image catalog is written to wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits -region wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.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.XSifKywnUT (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-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.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-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits
Checking if the catalog wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.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-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits
WCS catalog name: wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=130, bad_region=1621, passed=6993
Got 6993 stars (including 5282 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits.wcscat
util/solve_plate_with_UCAC5 got 6993 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 5520 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 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 5519 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 5519 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 949 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits N_match=949 sigma_overall_arcsec=0.475 sigma_q1_arcsec=0.477 sigma_q2_arcsec=0.433 sigma_q3_arcsec=0.681 sigma_q4_arcsec=0.437 n_q1=318 n_q2=260 n_q3=125 n_q4=246 worst_quadrant_to_overall_ratio=1.432
The image catalog is written to wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits -region wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.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.sIpphf4CYW (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-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.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-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
Checking if the catalog wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.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-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
WCS catalog name: wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=170, bad_region=1668, passed=6989
Got 6989 stars (including 5186 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits.wcscat
util/solve_plate_with_UCAC5 got 6989 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 5545 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 5544 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 5544 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 950 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits N_match=950 sigma_overall_arcsec=0.481 sigma_q1_arcsec=0.477 sigma_q2_arcsec=0.482 sigma_q3_arcsec=0.632 sigma_q4_arcsec=0.452 n_q1=302 n_q2=260 n_q3=142 n_q4=246 worst_quadrant_to_overall_ratio=1.314
The image catalog is written to wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits -region wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.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-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.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-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-22-28_20.00sec_5.00C_LIGHT_0348.fits
Saving fully-calibrated image wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.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-03-Q2b1x1_040502_TTUQ2b1x1_2769130_rTQUTVTL/wcs_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349.fits
Preparing the HTML report for the field Psc-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:43:06.03 +12:34:13.2: 12.64 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:53:00.35 +17:25:30.6: 12.88 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:53:03.57 +16:33:15.8: 13.22 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:53:26.30 +17:58:06.3: 12.85 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:38:14.13 +10:01:42.7: 12.90 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:50:24.63 +10:19:56.3: 12.69 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:53:07.24 +17:28:29.1: 13.00 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:54:40.28 +17:56:29.4: 13.46 +/- 0.03 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:52:38.19 +17:25:45.7: 12.98 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:40:38.50 +09:56:13.9: 13.38 +/- 0.03 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:43:06.03 +12:34:13.2: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Forced photometry filter REJECTED candidate at 01:43:06.03 +12:34:13.2: ref_mag=12.62 +/- 0.01 new_mean_mag=11.9086 delta=0.72 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:53:00.35 +17:25:30.6: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Forced photometry filter KEPT candidate at 01:53:00.35 +17:25:30.6: ref_mag=12.90 +/- 0.01 new_mean_mag=11.9828 delta=0.91 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:53:03.57 +16:33:15.8: 13.27 +/- 0.03 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:53:26.30 +17:58:06.3: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:50:24.63 +10:19:56.3: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Forced photometry filter KEPT candidate at 01:53:26.30 +17:58:06.3: ref_mag=12.86 +/- 0.01 new_mean_mag=11.9124 delta=0.95 (need > 0.90)
Forced photometry filter KEPT candidate at 01:53:03.57 +16:33:15.8: ref_mag=13.24 +/- 0.02 new_mean_mag=12.1389 delta=1.10 (need > 0.90)
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Forced photometry filter REJECTED candidate at 01:50:24.63 +10:19:56.3: ref_mag=12.67 +/- 0.01 new_mean_mag=12.0144 delta=0.65 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:54:40.28 +17:56:29.4: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.02
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:40:38.50 +09:56:13.9: 13.30 +/- 0.03 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:52:38.19 +17:25:45.7: 13.01 +/- 0.02 detection
Forced photometry filter KEPT candidate at 01:54:40.28 +17:56:29.4: ref_mag=13.45 +/- 0.02 new_mean_mag=12.3300 delta=1.12 (need > 0.90)
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Forced photometry reference-image weighted average: 12.99 +/- 0.01
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:53:07.24 +17:28:29.1: 13.00 +/- 0.02 detection
Forced photometry filter KEPT candidate at 01:40:38.50 +09:56:13.9: ref_mag=13.35 +/- 0.02 new_mean_mag=12.2374 delta=1.11 (need > 0.90)
Forced photometry filter KEPT candidate at 01:52:38.19 +17:25:45.7: ref_mag=12.99 +/- 0.01 new_mean_mag=11.9932 delta=1.00 (need > 0.90)
Forced photometry reference-image weighted average: 13.00 +/- 0.01
Forced photometry filter KEPT candidate at 01:53:07.24 +17:28:29.1: ref_mag=13.00 +/- 0.01 new_mean_mag=12.0724 delta=0.93 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:38:14.13 +10:01:42.7: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Forced photometry filter KEPT candidate at 01:38:14.13 +10:01:42.7: ref_mag=12.91 +/- 0.02 new_mean_mag=11.8675 delta=1.04 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:52:20.08 +17:12:35.0: 12.86 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:52:51.74 +17:20:15.7: 12.85 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:52:20.08 +17:12:35.0: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.01
Forced photometry filter KEPT candidate at 01:52:20.08 +17:12:35.0: ref_mag=12.87 +/- 0.01 new_mean_mag=11.7693 delta=1.10 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:52:51.74 +17:20:15.7: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
Forced photometry filter KEPT candidate at 01:52:51.74 +17:20:15.7: ref_mag=12.88 +/- 0.01 new_mean_mag=11.9557 delta=0.92 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:50:46.84 +17:01:56.7: 13.17 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:53:43.26 +18:00:34.9: 13.35 +/- 0.03 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:38:23.04 +09:47:53.0: 12.56 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:42:41.08 +12:26:36.9: 13.13 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:54:19.91 +17:55:44.4: 13.13 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:50:46.84 +17:01:56.7: 13.17 +/- 0.03 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:53:43.26 +18:00:34.9: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:38:23.04 +09:47:53.0: 12.48 +/- 0.02 detection
Forced photometry filter KEPT candidate at 01:50:46.84 +17:01:56.7: ref_mag=13.17 +/- 0.02 new_mean_mag=12.1622 delta=1.01 (need > 0.90)
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Forced photometry filter KEPT candidate at 01:53:43.26 +18:00:34.9: ref_mag=13.37 +/- 0.02 new_mean_mag=12.2879 delta=1.08 (need > 0.90)
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Forced photometry filter KEPT candidate at 01:38:23.04 +09:47:53.0: ref_mag=12.52 +/- 0.01 new_mean_mag=11.5893 delta=0.93 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:42:41.08 +12:26:36.9: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 01:42:41.08 +12:26:36.9: ref_mag=13.14 +/- 0.02 new_mean_mag=12.1458 delta=1.00 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:54:19.91 +17:55:44.4: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 01:54:19.91 +17:55:44.4: ref_mag=13.14 +/- 0.02 new_mean_mag=12.1258 delta=1.02 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:37:38.76 +09:43:20.3: 12.75 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:52:24.63 +17:07:12.8: 13.11 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:37:38.76 +09:43:20.3: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Forced photometry filter KEPT candidate at 01:37:38.76 +09:43:20.3: ref_mag=12.76 +/- 0.01 new_mean_mag=11.7786 delta=0.98 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:39:59.21 +11:09:59.4: 12.71 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:52:24.63 +17:07:12.8: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry filter KEPT candidate at 01:52:24.63 +17:07:12.8: ref_mag=13.10 +/- 0.02 new_mean_mag=12.1558 delta=0.95 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:39:59.21 +11:09:59.4: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Forced photometry filter KEPT candidate at 01:39:59.21 +11:09:59.4: ref_mag=12.70 +/- 0.01 new_mean_mag=11.7377 delta=0.96 (need > 0.90)
Adding exclusion_list_local.txt__out05163.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05320.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05432.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05492.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07374.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07545.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07565.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07938.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08478.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08844.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09202.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11102.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28892.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29204.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29825.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30326.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34963.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40112.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 39s
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: 15s
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Considering the candidate 51261_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349
The candidate 51261_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349 did not pass the final checks
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Considering the candidate 29825_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349
Preparing report for the candidate 29825_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349
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Considering the candidate 11102_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349
Preparing report for the candidate 11102_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349
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Considering the candidate 05432_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349
Preparing report for the candidate 05432_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349
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Considering the candidate 05320_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349
Preparing report for the candidate 05320_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349
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Considering the candidate 07565_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349
Preparing report for the candidate 07565_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349
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Considering the candidate 30326_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349
Preparing report for the candidate 30326_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349
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Considering the candidate 07545_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349
Preparing report for the candidate 07545_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349
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Considering the candidate 07374_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349
Preparing report for the candidate 07374_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349
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Considering the candidate 31420_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349
The candidate 31420_fd_Psc-03-Q2b1x1_2026-07-10_03-23-15_20.00sec_5.00C_LIGHT_0349 did not pass the final checks
