This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
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,2461231.8947,7.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260710.3947 7.08CV 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 10.3947 2461231.8947 9.66 01:17:22.21 +03:10:03.9
135.60000 -59.06469 galactic Psc Second-epoch detections are separated by 0.5" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.2 Pallas 0 -1 1 9.8 0 0
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 01:17:22.21 +03:10:03.9: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 01:17:22.21 +03:10:03.9: 15.67 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461231.8947,9.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260710.3947 9.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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,2461231.8947,7.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260710.3947 7.47CV 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 10.3947 2461231.8947 12.53 00:45:12.69 +03:48:22.0
119.91269 -59.02913 galactic Psc Second-epoch detections are separated by 1.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.2323 Zverev -60 -54 81 17.1 0 0
ATTENTION: measured mag 12.53 is 4.6 mag brighter than the predicted asteroid brightness 17.1 - the transient may be an unrelated new object!
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:45:12.69 +03:48:22.0: 13.59 +/- 0.04 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:45:12.69 +03:48:22.0: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461231.8947,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260710.3947 12.53CV 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 10.3947 2461231.8947 12.87 00:44:32.62 +03:09:58.3
119.52352 -59.65992 galactic Psc Second-epoch detections are separated by 1.7" and 7.0 pix
The object was found in VSX 1" ASASSN-V J004432.57+030959.1
Type: ROT
# Max. Min./Amp. JD0 Period
14.060 V 14.150 V 2458011.92300 1.141150000000
The object was not found in astcheck.
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:44:32.62 +03:09:58.3: 13.94 +/- 0.05 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:44:32.62 +03:09:58.3: 13.93 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J004432.57+030959.1,2461231.8947,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J004432.57+030959.1 20260710.3947 12.87CV 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 10.3947 2461231.8947 12.80 00:55:17.88 +05:25:21.4
124.71700 -57.43576 galactic Psc Second-epoch detections are separated by 2.0" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:55:17.88 +05:25:21.4 (user input) | T | P | (position from user input) J-Ks=0.684+/-0.033 (K)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:55:17.88 +05:25:21.4: 13.69 +/- 0.04 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:55:17.88 +05:25:21.4: 13.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461231.8947,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3947 12.80CV 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 10.3947 2461231.8947 12.80 00:46:44.47 +04:11:07.1
120.67958 -58.66590 galactic Psc Second-epoch detections are separated by 3.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:46:44.47 +04:11:07.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.563+/-0.033 (K)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:46:44.47 +04:11:07.1: 13.90 +/- 0.05 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:46:44.47 +04:11:07.1: 13.89 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461231.8947,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3947 12.80CV 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 10.3947 2461231.8947 12.80 00:44:39.77 +04:07:13.7
119.67801 -58.70847 galactic Psc Second-epoch detections are separated by 1.2" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:44:39.77 +04:07:13.7 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.390+/-0.038 (G)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:44:39.77 +04:07:13.7: 13.85 +/- 0.05 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:44:39.77 +04:07:13.7: 13.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461231.8947,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3947 12.80CV 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 10.3947 2461231.8947 12.76 00:55:49.80 +05:31:09.6
124.95719 -57.33514 galactic Psc Second-epoch detections are separated by 0.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:55:49.80 +05:31:09.6 (user input) | T | P | (position from user input) J-Ks=0.460+/-0.037 (G)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:55:49.80 +05:31:09.6: 13.84 +/- 0.05 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:55:49.80 +05:31:09.6: 13.83 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461231.8947,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3947 12.76CV 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 10.3947 2461231.8947 12.21 00:26:18.56 +09:52:23.1
112.73169 -52.50028 galactic Psc Second-epoch detections are separated by 1.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:26:18.56 +09:52:23.1 (user input) | T | P | (position from user input) J-Ks=0.460+/-0.032 (G)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:26:18.56 +09:52:23.1: 13.30 +/- 0.04 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:26:18.56 +09:52:23.1: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461231.8947,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3947 12.21CV 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 10.3947 2461231.8947 12.67 00:44:58.09 +03:44:56.5
119.78946 -59.08324 galactic Psc Second-epoch detections are separated by 1.1" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.2323 Zverev -278 -260 381 17.1 0 0
ATTENTION: measured mag 12.67 is 4.4 mag brighter than the predicted asteroid brightness 17.1 - the transient may be an unrelated new object!
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:44:58.09 +03:44:56.5: 13.67 +/- 0.04 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:44:58.09 +03:44:56.5: 13.72 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461231.8947,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260710.3947 12.67CV 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 10.3947 2461231.8947 12.09 00:30:36.87 +10:56:09.0
114.68557 -51.60219 galactic Psc Second-epoch detections are separated by 2.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 2751528299481122688 | 00:30:36.87 +10:56:09.0 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.117+/-0.034 (A)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:30:36.87 +10:56:09.0: 12.99 +/- 0.03 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:30:36.87 +10:56:09.0: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 2751528299481122688,2461231.8947,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 2751528299481122688 20260710.3947 12.09CV 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 10.3947 2461231.8947 12.80 00:50:56.77 +04:39:24.4
122.69929 -58.21475 galactic Psc Second-epoch detections are separated by 2.5" and 7.2 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 | 00:50:56.77 +04:39:24.4 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.551+/-0.034 (K)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:50:56.77 +04:39:24.4: 13.75 +/- 0.04 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:50:56.77 +04:39:24.4: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461231.8947,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3947 12.80CV 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 10.3947 2461231.8947 12.40 00:55:25.24 +05:03:06.9
124.79369 -57.80543 galactic Psc Second-epoch detections are separated by 0.5" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:55:25.24 +05:03:06.9 (user input) | T | P | (position from user input) J-Ks=0.446+/-0.039 (G)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:55:25.24 +05:03:06.9: 13.22 +/- 0.03 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:55:25.24 +05:03:06.9: 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!
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,2461231.8947,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3947 12.40CV 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 10.3947 2461231.8947 12.77 00:52:37.33 +04:19:27.7
123.49768 -58.54609 galactic Psc Second-epoch detections are separated by 2.9" and 6.9 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 | 00:52:37.33 +04:19:27.7 (user input) | T | P | (position from user input) J-Ks=0.546+/-0.032 (K)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:52:37.33 +04:19:27.7: 13.76 +/- 0.04 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:52:37.33 +04:19:27.7: 13.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461231.8947,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3947 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3947 2461231.8947 12.61 00:45:09.78 +03:37:59.9
119.87323 -59.20117 galactic Psc Second-epoch detections are separated by 1.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:45:09.78 +03:37:59.9 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.347+/-0.037 (G)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:45:09.78 +03:37:59.9: 13.51 +/- 0.04 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:45:09.78 +03:37:59.9: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461231.8947,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3947 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3947 2461231.8947 12.54 00:45:34.08 +04:02:52.2
120.10600 -58.79170 galactic Psc Second-epoch detections are separated by 2.8" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:45:34.08 +04:02:52.2 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:45:34.08 +04:02:52.2: 13.51 +/- 0.04 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:45:34.08 +04:02:52.2: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 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,2461231.8947,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3947 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3947 2461231.8947 12.61 00:43:26.63 +03:48:52.0
119.05833 -58.99717 galactic Psc Second-epoch detections are separated by 1.2" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1998 Titius 91 -337 349 17.0 0 0
ATTENTION: measured mag 12.61 is 4.4 mag brighter than the predicted asteroid brightness 17.0 - the transient may be an unrelated new object!
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:43:26.63 +03:48:52.0: 13.49 +/- 0.04 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:43:26.63 +03:48:52.0: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461231.8947,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260710.3947 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3947 2461231.8947 12.55 00:56:17.56 +04:52:45.2
125.21253 -57.97103 galactic Psc Second-epoch detections are separated by 0.8" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.2230 Yunnan 278 -291 402 17.4 0 0
ATTENTION: measured mag 12.55 is 4.8 mag brighter than the predicted asteroid brightness 17.4 - the transient may be an unrelated new object!
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:56:17.56 +04:52:45.2: 13.45 +/- 0.03 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:56:17.56 +04:52:45.2: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 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
VARIABLE_NAME,2461231.8947,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260710.3947 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3947 2461231.8947 12.26 00:26:16.53 +09:50:36.9
112.71041 -52.52807 galactic Psc Second-epoch detections are separated by 1.1" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:26:16.53 +09:50:36.9 (user input) | T | P | (position from user input) J-Ks=0.724+/-0.032 (K)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:26:16.53 +09:50:36.9: 13.38 +/- 0.04 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:26:16.53 +09:50:36.9: 13.33 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461231.8947,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3947 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 10.3947 2461231.8947 12.24 00:29:46.96 +11:01:35.0
114.37948 -51.48540 galactic Psc Second-epoch detections are separated by 0.8" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:29:46.96 +11:01:35.0 (user input) | T | P | (position from user input) J-Ks=0.384+/-0.034 (G)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:29:46.96 +11:01:35.0: 13.15 +/- 0.03 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:29:46.96 +11:01:35.0: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 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,2461231.8947,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3947 12.24CV 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 10.3947 2461231.8947 11.98 00:26:40.17 +10:36:07.7
113.06152 -51.79430 galactic Psc Second-epoch detections are separated by 1.5" and 6.9 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 | 00:26:40.17 +10:36:07.7 (user input) | T | P | (position from user input) J-Ks=0.364+/-0.033 (G)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:26:40.17 +10:36:07.7: 12.87 +/- 0.02 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:26:40.17 +10:36:07.7: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461231.8947,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3947 11.98CV 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 10.3947 2461231.8947 12.94 00:53:27.71 +05:58:54.9
123.85309 -56.88621 galactic Psc Second-epoch detections are separated by 2.4" and 6.9 pix
The object was found in VSX23" Gaia DR3 2553318135751667584
Type: ROT
# Max. Min./Amp. JD0 Period
14.860 G 14.890 G K
The object was not found in astcheck.
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:53:27.71 +05:58:54.9: 13.93 +/- 0.05 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:53:27.71 +05:58:54.9: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2553318135751667584,2461231.8947,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2553318135751667584 20260710.3947 12.94CV 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 10.3947 2461231.8947 12.91 00:45:04.53 +04:00:01.4
119.86486 -58.83347 galactic Psc Second-epoch detections are separated by 0.8" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:45:04.53 +04:00:01.4 (user input) | T | P | (position from user input) J-Ks=0.357+/-0.035 (G)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:45:04.53 +04:00:01.4: 13.90 +/- 0.05 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:45:04.53 +04:00:01.4: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.8947,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3947 12.91CV 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: 2461049.62262976 09.01.2026 02:56:25.211 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
First image: 2461049.62262976 09.01.2026 02:56:25.211 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
Last image: 2461231.89499773 10.07.2026 09:28:37.804 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.65
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 7 seconds
Number of parallel threads: 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): 5905
Objects passed selection criteria: 5876
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 3878.25
Average stars matched: 3783 (97.544 %)
Memory usage VmPeak: 112172 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 04:50:28 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: 2461049.62262976 09.01.2026 02:56:25.211 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
First image: 2461049.62262976 09.01.2026 02:56:25.211 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
Last image: 2461231.89499773 10.07.2026 09:28:37.804 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 37
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.42
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: 16 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): 31920
Objects passed selection criteria: 31827
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 21668
Average stars matched: 20982 (96.834 %)
Memory usage VmPeak: 135060 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 04:53:19 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
SExtractor catalog cache: saved Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.cat to cache
SExtractor catalog cache: saved Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.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-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.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: 2461231.89436918
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-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits exists and is non-empty
Saving wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits to local_wcs_cache/
'wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits' -> 'local_wcs_cache/wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits'
wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits exists and is non-empty
Saving wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits to local_wcs_cache/
'wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits' -> 'local_wcs_cache/wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits'
wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits exists and is non-empty
Saving wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits to local_wcs_cache/
'wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits' -> 'local_wcs_cache/wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits'
wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits exists and is non-empty
Saving wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits to local_wcs_cache/
'wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits' -> 'local_wcs_cache/wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits (1st reference image)
verification OK: wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:51:32.310 +05:59:46.72 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-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits (1st new image)
verification OK: wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits
Image size: 941.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:51:47.277 +05:58:54.34 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:51:32.310 +05:59:46.72
Second-epoch image center 00:51:47.277 +05:58:54.34
Angular distance between the image centers 0.0637 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits (2nd new image)
verification OK: wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
Image size: 941.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:51:44.996 +05:59:16.23 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:51:32.310 +05:59:46.72
Second-epoch image center 00:51:44.996 +05:59:16.23
Angular distance between the image centers 0.0532 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 00:51:47.277 +05:58:54.34
Second-epoch second image center 00:51:44.996 +05:59:16.23
Angular distance between the image centers 0.01124 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-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits &> /tmp/tmp.5Xi2RXx5Yb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits &> /tmp/tmp.1ZSIJF19As
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits &> /tmp/tmp.04cuBRVfPB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits &> /tmp/tmp.72gmiF78uK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.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-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits and wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.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-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits and wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat
Found non-empty wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits and wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat
The reference image (wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits) and catalog (wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat) found
'wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat' -> 'wcsmag.cat'
Read 6274 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 4.9081 to 20.8681 deg, Dec +0.7095 to +11.2754 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 4.9081 to 20.8681 deg, Dec 0.7095 to 11.2754 deg
Loaded 4466 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): 3642 out of 3799 total matches.
Matched with Tycho-2 3799 out of 6274 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.877250
a=0.000000 b=1.000000 c=22.877250
From vast_summary.log: estimated ref. image limiting mag.: -7.65
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.23
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.23
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6274 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 4.9081 to 20.8681 deg, Dec +0.7095 to +11.2754 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 4.9081 to 20.8681 deg, Dec 0.7095 to 11.2754 deg
Loaded 4466 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): 3642 out of 3799 total matches.
Matched with Tycho-2 3799 out of 6274 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits:
Forced-photometry filter: calibrated wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits -> calib.txt_param_ref_wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits (aperture=5.9)
Read 6217 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 4.8906 to 20.8646 deg, Dec +0.7094 to +11.2737 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 4.8906 to 20.8646 deg, Dec 0.7094 to 11.2737 deg
Loaded 4467 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): 3635 out of 3795 total matches.
Matched with Tycho-2 3795 out of 6217 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits:
Forced-photometry filter: calibrated wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits -> calib.txt_param_ref_wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
2.0 pix Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
3.1 pix fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits
3.0 pix fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
2.0 pix wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
2.0 pix wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
Limiting magnitude estimates:
15.2 mag. Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
15.2 mag. Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
13.2 mag. fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits
13.0 mag. fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
All-image limiting magnitude estimate: 13.0 (SNR ) 10.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.5Xi2RXx5Yb (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.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-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits' -> 'wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
WCS_IMAGE_NAME=wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
WCS-calibrated image found: wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
Checking if the catalog wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat corresponding to the image wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits alredy exist and is non-empty...
Catalog wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat corresponding to the image wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
WCS catalog name: wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=428, bad_region=0, passed=6274
Got 6274 stars (including 5838 good ones) from the SExtractor catalog wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat
util/solve_plate_with_UCAC5 got 6274 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 6184 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 6184 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 6184 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits N_match=979 sigma_overall_arcsec=0.291 sigma_q1_arcsec=0.359 sigma_q2_arcsec=0.275 sigma_q3_arcsec=0.267 sigma_q4_arcsec=0.273 n_q1=207 n_q2=265 n_q3=258 n_q4=249 worst_quadrant_to_overall_ratio=1.235
The image catalog is written to wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits -region wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.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.1ZSIJF19As (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.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-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits' -> 'wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
WCS_IMAGE_NAME=wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
WCS-calibrated image found: wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
Checking if the catalog wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat corresponding to the image wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits alredy exist and is non-empty...
Catalog wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat corresponding to the image wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
WCS catalog name: wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=435, bad_region=0, passed=6217
Got 6217 stars (including 5773 good ones) from the SExtractor catalog wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat
util/solve_plate_with_UCAC5 got 6217 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 6112 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 6111 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 6111 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 980 stars left (next iteration limit 1078)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits N_match=980 sigma_overall_arcsec=0.288 sigma_q1_arcsec=0.400 sigma_q2_arcsec=0.286 sigma_q3_arcsec=0.253 sigma_q4_arcsec=0.236 n_q1=208 n_q2=264 n_q3=255 n_q4=253 worst_quadrant_to_overall_ratio=1.387
The image catalog is written to wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits -region wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.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.04cuBRVfPB (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-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.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-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits
WCS_IMAGE_NAME=wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits
WCS-calibrated image found: wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits
Checking if the catalog wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits.wcscat corresponding to the image wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits.wcscat corresponding to the image wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.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-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits
WCS catalog name: wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=81, bad_region=0, passed=1651
Got 1651 stars (including 1569 good ones) from the SExtractor catalog wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits.wcscat
util/solve_plate_with_UCAC5 got 1651 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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 451 to 509 (Dec 0.4 to 11.6)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 1591 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 451 to 509 (Dec 0.4 to 11.6)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 1589 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 1589 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits N_match=977 sigma_overall_arcsec=0.294 sigma_q1_arcsec=0.304 sigma_q2_arcsec=0.297 sigma_q3_arcsec=0.288 sigma_q4_arcsec=0.283 n_q1=273 n_q2=377 n_q3=132 n_q4=195 worst_quadrant_to_overall_ratio=1.035
The image catalog is written to wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits -region wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.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.72gmiF78uK (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-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.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-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
WCS_IMAGE_NAME=wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
WCS-calibrated image found: wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
Checking if the catalog wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits.wcscat corresponding to the image wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits.wcscat corresponding to the image wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.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-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
WCS catalog name: wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=77, bad_region=0, passed=1466
Got 1466 stars (including 1389 good ones) from the SExtractor catalog wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits.wcscat
util/solve_plate_with_UCAC5 got 1466 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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 451 to 509 (Dec 0.4 to 11.6)
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(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 1424 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 451 to 509 (Dec 0.4 to 11.6)
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(), 1426 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 1426 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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=fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits N_match=974 sigma_overall_arcsec=0.297 sigma_q1_arcsec=0.278 sigma_q2_arcsec=0.318 sigma_q3_arcsec=0.287 sigma_q4_arcsec=0.302 n_q1=244 n_q2=373 n_q3=179 n_q4=178 worst_quadrant_to_overall_ratio=1.070
The image catalog is written to wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits -region wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.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-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits sigma_overall=0.291 worst_q_ratio=1.235
ref2=Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits sigma_overall=0.288 worst_q_ratio=1.387
new1=fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits sigma_overall=0.294 worst_q_ratio=1.035
new2=fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits sigma_overall=0.297 worst_q_ratio=1.070
reference average sigma_overall=0.2895 worst_q_ratio=1.311
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069_astrometric_residuals.png (979 matched stars from wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070_astrometric_residuals.png (980 matched stars from wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370_astrometric_residuals.png (977 matched stars from wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371_astrometric_residuals.png (974 matched stars from wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits'
Saving fully-calibrated image wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits'
Preparing the HTML report for the field Psc-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 01:17:22.21 +03:10:03.9: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 01:17:22.21 +03:10:03.9: 15.67 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out20329.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
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: 3s
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Considering the candidate 20320_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
Preparing report for the candidate 20320_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20329_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
Preparing report for the candidate 20329_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01357_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
The candidate 01357_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371 did not pass the final checks
**** FOUND 01:17:34.24 +08:55:51.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 13s
Prepared the HTML report for the field Psc-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
01:17:22.21 +03:10:03.9
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
SExtractor catalog cache: saved Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.cat to cache
SExtractor catalog cache: saved Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.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-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
Creating symlink local_wcs_cache/wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits exists and is non-empty
wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits exists and is non-empty
wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits exists and is non-empty
wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits (1st reference image)
verification OK: wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:51:32.310 +05:59:46.72 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-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits (1st new image)
verification OK: wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits
Image size: 941.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:51:47.277 +05:58:54.34 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:51:32.310 +05:59:46.72
Second-epoch image center 00:51:47.277 +05:58:54.34
Angular distance between the image centers 0.0637 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits (2nd new image)
verification OK: wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
Image size: 941.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:51:44.996 +05:59:16.23 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:51:32.310 +05:59:46.72
Second-epoch image center 00:51:44.996 +05:59:16.23
Angular distance between the image centers 0.0532 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 00:51:47.277 +05:58:54.34
Second-epoch second image center 00:51:44.996 +05:59:16.23
Angular distance between the image centers 0.01124 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-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits &> /tmp/tmp.FyDSw79R0m
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits &> /tmp/tmp.Vr51p1USXB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits &> /tmp/tmp.6Mt198k45H
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits &> /tmp/tmp.LBYyL1mC5j
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.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-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits and wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.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-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits and wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat
Found non-empty wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits and wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat
The reference image (wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits) and catalog (wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat) found
'wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat' -> 'wcsmag.cat'
Read 34129 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 4.8906 to 20.8698 deg, Dec +0.7073 to +11.2841 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 4.8906 to 20.8698 deg, Dec 0.7073 to 11.2841 deg
Loaded 4478 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): 3588 out of 3910 total matches.
Matched with Tycho-2 3910 out of 34129 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.782000
a=0.000000 b=1.000000 c=22.782000
From vast_summary.log: estimated ref. image limiting mag.: -7.42
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.36
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.36
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 34129 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 4.8906 to 20.8698 deg, Dec +0.7073 to +11.2841 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 4.8906 to 20.8698 deg, Dec 0.7073 to 11.2841 deg
Loaded 4478 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): 3588 out of 3910 total matches.
Matched with Tycho-2 3910 out of 34129 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits:
Forced-photometry filter: calibrated wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits -> calib.txt_param_ref_wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits (aperture=4.8)
Read 34111 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 4.8822 to 20.8645 deg, Dec +0.7037 to +11.2806 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 4.8822 to 20.8645 deg, Dec 0.7037 to 11.2806 deg
Loaded 4474 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): 3580 out of 3908 total matches.
Matched with Tycho-2 3908 out of 34111 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits:
Forced-photometry filter: calibrated wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits -> calib.txt_param_ref_wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 30 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
1.9 pix Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
2.8 pix fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits
2.8 pix fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
1.9 pix wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
1.9 pix wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
Limiting magnitude estimates:
15.4 mag. Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
15.4 mag. Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
13.3 mag. fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits
13.2 mag. fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 12.8 (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.FyDSw79R0m (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.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-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits' -> 'wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
WCS_IMAGE_NAME=wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
WCS-calibrated image found: wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
Checking if the catalog wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat corresponding to the image wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits alredy exist and is non-empty...
Catalog wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat corresponding to the image wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
WCS catalog name: wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=1306, bad_region=1, passed=34109
Got 34109 stars (including 32754 good ones) from the SExtractor catalog wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat
util/solve_plate_with_UCAC5 got 34109 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 33583 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 33584 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 33584 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits N_match=979 sigma_overall_arcsec=0.282 sigma_q1_arcsec=0.374 sigma_q2_arcsec=0.261 sigma_q3_arcsec=0.272 sigma_q4_arcsec=0.248 n_q1=210 n_q2=257 n_q3=258 n_q4=254 worst_quadrant_to_overall_ratio=1.325
The image catalog is written to wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits -region wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.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.Vr51p1USXB (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.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-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits' -> 'wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
WCS_IMAGE_NAME=wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
WCS-calibrated image found: wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
Checking if the catalog wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat corresponding to the image wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits alredy exist and is non-empty...
Catalog wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat corresponding to the image wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
WCS catalog name: wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=26, blended=1297, bad_region=1, passed=34085
Got 34085 stars (including 32720 good ones) from the SExtractor catalog wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat
util/solve_plate_with_UCAC5 got 34085 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 969 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 33452 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 33454 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 33454 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 980 stars left (next iteration limit 1078)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits N_match=980 sigma_overall_arcsec=0.288 sigma_q1_arcsec=0.390 sigma_q2_arcsec=0.254 sigma_q3_arcsec=0.249 sigma_q4_arcsec=0.255 n_q1=213 n_q2=257 n_q3=253 n_q4=257 worst_quadrant_to_overall_ratio=1.355
The image catalog is written to wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits -region wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.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.6Mt198k45H (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-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.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-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits
WCS_IMAGE_NAME=wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits
WCS-calibrated image found: wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits
Checking if the catalog wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits.wcscat corresponding to the image wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits.wcscat corresponding to the image wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.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-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits
WCS catalog name: wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=243, bad_region=1, passed=9979
Got 9979 stars (including 9717 good ones) from the SExtractor catalog wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits.wcscat
util/solve_plate_with_UCAC5 got 9979 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 9512 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 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 9512 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 9512 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits N_match=978 sigma_overall_arcsec=0.290 sigma_q1_arcsec=0.294 sigma_q2_arcsec=0.302 sigma_q3_arcsec=0.283 sigma_q4_arcsec=0.278 n_q1=276 n_q2=376 n_q3=135 n_q4=191 worst_quadrant_to_overall_ratio=1.041
The image catalog is written to wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits -region wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.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.LBYyL1mC5j (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-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.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-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
WCS_IMAGE_NAME=wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
WCS-calibrated image found: wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
Checking if the catalog wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits.wcscat corresponding to the image wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits.wcscat corresponding to the image wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.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-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
WCS catalog name: wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=182, bad_region=2, passed=9059
Got 9059 stars (including 8858 good ones) from the SExtractor catalog wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits.wcscat
util/solve_plate_with_UCAC5 got 9059 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 8794 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 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 8789 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 8789 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits N_match=976 sigma_overall_arcsec=0.283 sigma_q1_arcsec=0.281 sigma_q2_arcsec=0.316 sigma_q3_arcsec=0.280 sigma_q4_arcsec=0.279 n_q1=247 n_q2=370 n_q3=181 n_q4=178 worst_quadrant_to_overall_ratio=1.117
The image catalog is written to wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Psc-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits -region wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.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-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.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-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-27-43_20.00sec_-0.00C_LIGHTs_0370.fits
Saving fully-calibrated image wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.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-05-Q1b1x1_042910_TTUQ1b1x1_700499_S1moo6h2/wcs_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371.fits
Preparing the HTML report for the field Psc-05-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:46:44.47 +04:11:07.1: 13.90 +/- 0.05 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:44:32.62 +03:09:58.3: 13.94 +/- 0.05 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:45:12.69 +03:48:22.0: 13.59 +/- 0.04 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:55:17.88 +05:25:21.4: 13.69 +/- 0.04 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:44:39.77 +04:07:13.7: 13.85 +/- 0.05 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:55:49.80 +05:31:09.6: 13.84 +/- 0.05 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:46:44.47 +04:11:07.1: 13.89 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.03
Forced photometry filter KEPT candidate at 00:46:44.47 +04:11:07.1: ref_mag=13.89 +/- 0.03 new_mean_mag=12.7909 delta=1.10 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:44:39.77 +04:07:13.7: 13.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.03
Forced photometry filter KEPT candidate at 00:44:39.77 +04:07:13.7: ref_mag=13.86 +/- 0.03 new_mean_mag=12.7837 delta=1.07 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:45:12.69 +03:48:22.0: 13.55 +/- 0.04 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:55:17.88 +05:25:21.4: 13.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Forced photometry filter KEPT candidate at 00:45:12.69 +03:48:22.0: ref_mag=13.57 +/- 0.03 new_mean_mag=12.5215 delta=1.05 (need > 0.90)
Forced photometry reference-image weighted average: 13.74 +/- 0.03
Forced photometry filter KEPT candidate at 00:55:17.88 +05:25:21.4: ref_mag=13.74 +/- 0.03 new_mean_mag=12.7808 delta=0.96 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:55:49.80 +05:31:09.6: 13.83 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.03
Forced photometry filter KEPT candidate at 00:55:49.80 +05:31:09.6: ref_mag=13.83 +/- 0.03 new_mean_mag=12.7526 delta=1.08 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:26:18.56 +09:52:23.1: 13.30 +/- 0.04 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:44:32.62 +03:09:58.3: 13.93 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.04
Forced photometry filter KEPT candidate at 00:44:32.62 +03:09:58.3: ref_mag=13.93 +/- 0.04 new_mean_mag=12.8480 delta=1.08 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:44:58.09 +03:44:56.5: 13.67 +/- 0.04 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:26:18.56 +09:52:23.1: 13.35 +/- 0.04 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:30:36.87 +10:56:09.0: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Forced photometry filter KEPT candidate at 00:26:18.56 +09:52:23.1: ref_mag=13.33 +/- 0.03 new_mean_mag=12.1695 delta=1.16 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:44:58.09 +03:44:56.5: 13.72 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.03
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:30:36.87 +10:56:09.0: 13.04 +/- 0.03 detection
Forced photometry filter KEPT candidate at 00:44:58.09 +03:44:56.5: ref_mag=13.69 +/- 0.03 new_mean_mag=12.6715 delta=1.02 (need > 0.90)
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Forced photometry filter KEPT candidate at 00:30:36.87 +10:56:09.0: ref_mag=13.01 +/- 0.02 new_mean_mag=12.0700 delta=0.94 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:50:56.77 +04:39:24.4: 13.75 +/- 0.04 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:50:56.77 +04:39:24.4: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.03
Forced photometry filter KEPT candidate at 00:50:56.77 +04:39:24.4: ref_mag=13.79 +/- 0.03 new_mean_mag=12.8029 delta=0.99 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:52:37.33 +04:19:27.7: 13.76 +/- 0.04 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:55:25.24 +05:03:06.9: 13.22 +/- 0.03 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:52:37.33 +04:19:27.7: 13.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.03
Forced photometry filter KEPT candidate at 00:52:37.33 +04:19:27.7: ref_mag=13.75 +/- 0.03 new_mean_mag=12.7619 delta=0.99 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:55:25.24 +05:03:06.9: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Forced photometry filter KEPT candidate at 00:55:25.24 +05:03:06.9: ref_mag=13.24 +/- 0.02 new_mean_mag=12.3243 delta=0.92 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:45:09.78 +03:37:59.9: 13.51 +/- 0.04 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:45:09.78 +03:37:59.9: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.03
Forced photometry filter KEPT candidate at 00:45:09.78 +03:37:59.9: ref_mag=13.52 +/- 0.03 new_mean_mag=12.6074 delta=0.92 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:45:34.08 +04:02:52.2: 13.51 +/- 0.04 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:45:34.08 +04:02:52.2: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Forced photometry filter KEPT candidate at 00:45:34.08 +04:02:52.2: ref_mag=13.50 +/- 0.02 new_mean_mag=12.5464 delta=0.95 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:56:17.56 +04:52:45.2: 13.45 +/- 0.03 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:43:26.63 +03:48:52.0: 13.49 +/- 0.04 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:43:26.63 +03:48:52.0: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Forced photometry filter KEPT candidate at 00:43:26.63 +03:48:52.0: ref_mag=13.49 +/- 0.03 new_mean_mag=12.5368 delta=0.95 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:56:17.56 +04:52:45.2: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.02
Forced photometry filter KEPT candidate at 00:56:17.56 +04:52:45.2: ref_mag=13.46 +/- 0.02 new_mean_mag=12.4754 delta=0.98 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:26:16.53 +09:50:36.9: 13.38 +/- 0.04 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:29:46.96 +11:01:35.0: 13.15 +/- 0.03 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:29:46.96 +11:01:35.0: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Forced photometry filter KEPT candidate at 00:29:46.96 +11:01:35.0: ref_mag=13.18 +/- 0.02 new_mean_mag=12.1826 delta=1.00 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:26:16.53 +09:50:36.9: 13.33 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Forced photometry filter KEPT candidate at 00:26:16.53 +09:50:36.9: ref_mag=13.35 +/- 0.03 new_mean_mag=12.2316 delta=1.12 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:56:41.10 +05:32:05.7: 13.32 +/- 0.03 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:56:41.10 +05:32:05.7: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Forced photometry filter REJECTED candidate at 00:56:41.10 +05:32:05.7: ref_mag=13.26 +/- 0.02 new_mean_mag=12.5322 delta=0.73 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:26:40.17 +10:36:07.7: 12.87 +/- 0.02 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:26:40.17 +10:36:07.7: 12.92 +/- 0.03 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:53:27.71 +05:58:54.9: 13.93 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Forced photometry filter KEPT candidate at 00:26:40.17 +10:36:07.7: ref_mag=12.89 +/- 0.02 new_mean_mag=11.9457 delta=0.95 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:53:27.71 +05:58:54.9: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.04
Forced photometry filter KEPT candidate at 00:53:27.71 +05:58:54.9: ref_mag=13.94 +/- 0.04 new_mean_mag=12.9199 delta=1.02 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:45:04.53 +04:00:01.4: 13.90 +/- 0.05 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:45:04.53 +04:00:01.4: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.04
Forced photometry filter KEPT candidate at 00:45:04.53 +04:00:01.4: ref_mag=13.93 +/- 0.04 new_mean_mag=12.8905 delta=1.04 (need > 0.90)
Adding exclusion_list_local.txt__out00626.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out00922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01982.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04203.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04422.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19174.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24176.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25832.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28883.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29234.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31183.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31599.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31696.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31766.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32342.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32490.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32923.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33328.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 44s
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: 27s
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Considering the candidate 52251_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
Preparing report for the candidate 52251_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
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Considering the candidate 52261_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
The candidate 52261_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371 did not pass the final checks
**** FOUND 01:17:22.21 +03:10:03.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 03142_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
The candidate 03142_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371 did not pass the final checks
**** FOUND 00:23:53.60 +10:13:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31766_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
Preparing report for the candidate 31766_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
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Considering the candidate 29234_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
Preparing report for the candidate 29234_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
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Considering the candidate 19529_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
Preparing report for the candidate 19529_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
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Considering the candidate 32923_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
Preparing report for the candidate 32923_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
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Considering the candidate 26375_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
The candidate 26375_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371 did not pass the final checks
**** FOUND 01:13:40.51 +02:09:39.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28883_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
Preparing report for the candidate 28883_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
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Considering the candidate 19174_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
Preparing report for the candidate 19174_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
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Considering the candidate 04203_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
Preparing report for the candidate 04203_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
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Considering the candidate 31599_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
Preparing report for the candidate 31599_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
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Considering the candidate 00922_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
Preparing report for the candidate 00922_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
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Considering the candidate 25832_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
Preparing report for the candidate 25832_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
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Considering the candidate 03445_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
The candidate 03445_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371 did not pass the final checks
**** FOUND 00:24:17.61 +10:07:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20850_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
Preparing report for the candidate 20850_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
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Considering the candidate 33328_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
Preparing report for the candidate 33328_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
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Considering the candidate 03258_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
The candidate 03258_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371 did not pass the final checks
**** FOUND 00:24:03.33 +10:10:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31183_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
Preparing report for the candidate 31183_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
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Considering the candidate 03913_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
The candidate 03913_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371 did not pass the final checks
**** FOUND 00:23:09.08 +09:57:35.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32490_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
Preparing report for the candidate 32490_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
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Considering the candidate 31696_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
Preparing report for the candidate 31696_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
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Considering the candidate 24176_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
Preparing report for the candidate 24176_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
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Considering the candidate 07254_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
The candidate 07254_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371 did not pass the final checks
**** FOUND 01:17:34.23 +08:55:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 04422_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
Preparing report for the candidate 04422_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
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Considering the candidate 00626_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
Preparing report for the candidate 00626_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
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Considering the candidate 19138_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371
The candidate 19138_fd_Psc-05-Q1b1x1_2026-07-10_04-28-37_20.00sec_0.00C_LIGHTs_0371 did not pass the final checks
