This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I
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,2461286.9368,7.12,0.05,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 20260903.4368 7.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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,2461286.9368,8.44,0.05,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 20260903.4368 8.44CV 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 09 03.4368 2461286.9368 9.18 00:38:41.40 +07:21:48.6
117.36405 -55.37037 galactic Psc Second-epoch detections are separated by 0.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.192 Nausikaa 1 1 1 9.2 -0 -0
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 00:38:41.40 +07:21:48.6: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 00:38:41.40 +07:21:48.6: 15.62 +/- 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,2461286.9368,9.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260903.4368 9.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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,2461286.9368,7.58,0.05,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 20260903.4368 7.58CV 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,2461286.9368,8.47,0.05,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 20260903.4368 8.47CV 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
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,2461286.9368,11.83,0.05,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 20260903.4368 11.83CV 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 09 03.4368 2461286.9368 13.65 00:37:34.74 +08:39:14.8
117.08945 -54.06035 galactic Psc Second-epoch detections are separated by 0.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.577 Rhea -0 0 0 13.8 -0 -0
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 00:37:34.74 +08:39:14.8: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 00:37:34.74 +08:39:14.8: 15.72 +/- 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,2461286.9368,13.65,0.05,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 20260903.4368 13.65CV 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 09 03.4368 2461286.9368 13.86 00:24:04.16 +02:30:44.5
109.31445 -59.63383 galactic Psc Second-epoch detections are separated by 1.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.551 Ortrud -1 0 1 14.1 -0 -0
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 00:24:04.16 +02:30:44.5: 15.46 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 00:24:04.16 +02:30:44.5: 15.48 +/- 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,2461286.9368,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260903.4368 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461242.90247090 21.07.2026 09:39:23.486 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
First image: 2461242.90247090 21.07.2026 09:39:23.486 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
Last image: 2461286.93709851 03.09.2026 10:29:15.311 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.63
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 5568
Objects passed selection criteria: 5560
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 4630.5
Average stars matched: 4539.75 (98.0402 %)
Memory usage VmPeak: 232036 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Sep 3 06:17:46 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: 2461242.90247090 21.07.2026 09:39:23.486 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
First image: 2461242.90247090 21.07.2026 09:39:23.486 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
Last image: 2461286.93709851 03.09.2026 10:29:15.311 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 42
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.38
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: 9 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 28607
Objects passed selection criteria: 28528
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 26375.5
Average stars matched: 25450.5 (96.493 %)
Memory usage VmPeak: 252024 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Sep 3 06:18:36 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
SExtractor catalog cache: saved Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits.cat to cache
SExtractor catalog cache: saved Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.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_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.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: 2461286.93641223
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_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits exists and is non-empty
wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits exists and is non-empty
wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits exists and is non-empty
wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits (1st reference image)
verification OK: wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
Image size: 937.4'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:51:26.391 +05:59:58.81 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits (1st new image)
verification OK: wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits
Image size: 941.4'x626.8' 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: 00:51:36.078 +06:01:36.24 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:51:26.391 +05:59:58.81
Second-epoch image center 00:51:36.078 +06:01:36.24
Angular distance between the image centers 0.0484 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits (2nd new image)
verification OK: wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
Image size: 941.4'x626.8' 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: 00:51:33.584 +06:02:00.50 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:51:26.391 +05:59:58.81
Second-epoch image center 00:51:33.584 +06:02:00.50
Angular distance between the image centers 0.0451 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 00:51:36.078 +06:01:36.24
Second-epoch second image center 00:51:33.584 +06:02:00.50
Angular distance between the image centers 0.01234 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_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits &> /tmp/tmp.lw27aKHaKE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits &> /tmp/tmp.lDtERwvwR3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits &> /tmp/tmp.eT69liRHoV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits &> /tmp/tmp.lFwwToektP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.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_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits and wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.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_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits and wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits.wcscat
Found non-empty wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits and wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits.wcscat
The reference image (wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits) and catalog (wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits.wcscat) found
'wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits.wcscat' -> 'wcsmag.cat'
Read 5718 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 4.8579 to 20.7702 deg, Dec +0.6752 to +11.2667 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 4.8579 to 20.7702 deg, Dec 0.6752 to 11.2667 deg
Loaded 4455 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): 3613 out of 3699 total matches.
Matched with Tycho-2 3699 out of 5718 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.625400
a=0.000000 b=1.000000 c=22.625400
From vast_summary.log: estimated ref. image limiting mag.: -7.63
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.00
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.00
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5718 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 4.8579 to 20.7702 deg, Dec +0.6752 to +11.2667 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 4.8579 to 20.7702 deg, Dec 0.6752 to 11.2667 deg
Loaded 4455 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): 3613 out of 3699 total matches.
Matched with Tycho-2 3699 out of 5718 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
Forced-photometry filter: calibrated wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits -> calib.txt_param_ref_wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits (aperture=6.4)
Read 5640 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 4.8902 to 20.7787 deg, Dec +0.7135 to +11.2815 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 4.8902 to 20.7787 deg, Dec 0.7135 to 11.2815 deg
Loaded 4441 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): 3584 out of 3667 total matches.
Matched with Tycho-2 3667 out of 5640 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits
Forced-photometry filter: calibrated wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits -> calib.txt_param_ref_wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits (aperture=6.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
2.3 pix Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits
2.1 pix fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits
2.1 pix fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
Limiting magnitude estimates:
15.0 mag. Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
15.0 mag. Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits
14.5 mag. fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits
14.5 mag. fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.lw27aKHaKE (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.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_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits' -> 'wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
WCS_IMAGE_NAME=wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
WCS-calibrated image found: wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
Checking if the catalog wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits.wcscat corresponding to the image wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits alredy exist and is non-empty...
Catalog wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits.wcscat corresponding to the image wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.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_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
WCS catalog name: wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.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=319, bad_region=0, passed=5718
Got 5718 stars (including 5395 good ones) from the SExtractor catalog wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits.wcscat
util/solve_plate_with_UCAC5 got 5718 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 4907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 5718 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 5718 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 5718 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4907 stars left (next iteration limit 5397)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits N_match=4907 sigma_overall_arcsec=0.327 sigma_q1_arcsec=0.292 sigma_q2_arcsec=0.366 sigma_q3_arcsec=0.331 sigma_q4_arcsec=0.335 n_q1=1254 n_q2=1243 n_q3=1220 n_q4=1190 worst_quadrant_to_overall_ratio=1.118
The image catalog is written to wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits -region wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.lDtERwvwR3 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.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_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits' -> 'wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits
WCS_IMAGE_NAME=wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits
WCS-calibrated image found: wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits
Checking if the catalog wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits.wcscat corresponding to the image wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits alredy exist and is non-empty...
Catalog wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits.wcscat corresponding to the image wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.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_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits
WCS catalog name: wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.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=319, bad_region=0, passed=5640
Got 5640 stars (including 5317 good ones) from the SExtractor catalog wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits.wcscat
util/solve_plate_with_UCAC5 got 5640 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4917 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4909 matched stars entering correct_measured_positions(), 4909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4909 matched stars entering correct_measured_positions(), 5640 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4917 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4908 matched stars entering correct_measured_positions(), 5640 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4908 matched stars entering correct_measured_positions(), 5640 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4908 stars left (next iteration limit 5399)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits N_match=4908 sigma_overall_arcsec=0.389 sigma_q1_arcsec=0.330 sigma_q2_arcsec=0.416 sigma_q3_arcsec=0.425 sigma_q4_arcsec=0.393 n_q1=1266 n_q2=1252 n_q3=1219 n_q4=1171 worst_quadrant_to_overall_ratio=1.093
The image catalog is written to wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits -region wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.eT69liRHoV (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_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.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_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits
WCS_IMAGE_NAME=wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits
WCS-calibrated image found: wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits
Checking if the catalog wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits.wcscat corresponding to the image wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits.wcscat corresponding to the image wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.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_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits
WCS catalog name: wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.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=282, bad_region=0, passed=3619
Got 3619 stars (including 3332 good ones) from the SExtractor catalog wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits.wcscat
util/solve_plate_with_UCAC5 got 3619 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.4 to 11.7)
Done reading UCAC5 zone files...
Matched 3280 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3277 matched stars entering correct_measured_positions(), 3278 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3277 matched stars entering correct_measured_positions(), 3619 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.4 to 11.7)
Done reading UCAC5 zone files...
Matched 3282 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3278 matched stars entering correct_measured_positions(), 3619 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 3278 matched stars entering correct_measured_positions(), 3619 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 3278 stars left (next iteration limit 3604)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3278 robust_rms=12.012 arcsec worst_quadrant_rms=12.595 arcsec
SIP_REFIT: SIP order 3 trial: matched=3278 robust_rms=0.494 arcsec worst_quadrant_rms=0.567 arcsec
SIP_REFIT: SIP order 5 trial: matched=3278 robust_rms=0.318 arcsec worst_quadrant_rms=0.376 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3278 robust_rms_before=1.004 arcsec robust_rms_before_corrected=0.334 arcsec robust_rms_after=0.318 arcsec worst_quadrant_rms_before=0.379 worst_quadrant_rms_after=0.376
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.379 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits N_match=3278 sigma_overall_arcsec=0.341 sigma_q1_arcsec=0.354 sigma_q2_arcsec=0.395 sigma_q3_arcsec=0.346 sigma_q4_arcsec=0.295 n_q1=723 n_q2=778 n_q3=900 n_q4=877 worst_quadrant_to_overall_ratio=1.156
The image catalog is written to wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits -region wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.lFwwToektP (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_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.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_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
WCS_IMAGE_NAME=wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
WCS-calibrated image found: wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
Checking if the catalog wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits.wcscat corresponding to the image wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits.wcscat corresponding to the image wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.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_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
WCS catalog name: wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.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=314, bad_region=0, passed=3661
Got 3661 stars (including 3343 good ones) from the SExtractor catalog wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits.wcscat
util/solve_plate_with_UCAC5 got 3661 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.4 to 11.7)
Done reading UCAC5 zone files...
Matched 3289 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3286 matched stars entering correct_measured_positions(), 3287 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3286 matched stars entering correct_measured_positions(), 3661 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.4 to 11.7)
Done reading UCAC5 zone files...
Matched 3290 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3287 matched stars entering correct_measured_positions(), 3661 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 3287 matched stars entering correct_measured_positions(), 3661 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 3287 stars left (next iteration limit 3614)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3287 robust_rms=11.707 arcsec worst_quadrant_rms=12.149 arcsec
SIP_REFIT: SIP order 3 trial: matched=3287 robust_rms=0.472 arcsec worst_quadrant_rms=0.579 arcsec
SIP_REFIT: SIP order 5 trial: matched=3287 robust_rms=0.318 arcsec worst_quadrant_rms=0.373 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3287 robust_rms_before=1.006 arcsec robust_rms_before_corrected=0.333 arcsec robust_rms_after=0.318 arcsec worst_quadrant_rms_before=0.372 worst_quadrant_rms_after=0.373
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.372 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits N_match=3287 sigma_overall_arcsec=0.347 sigma_q1_arcsec=0.343 sigma_q2_arcsec=0.381 sigma_q3_arcsec=0.356 sigma_q4_arcsec=0.301 n_q1=734 n_q2=783 n_q3=903 n_q4=867 worst_quadrant_to_overall_ratio=1.098
The image catalog is written to wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits -region wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits to local_wcs_cache/
'wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits' -> 'local_wcs_cache/wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits'
Saving the final (post-refit) wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits to local_wcs_cache/
'wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits' -> 'local_wcs_cache/wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits'
Saving the final (post-refit) wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits to local_wcs_cache/
'wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits' -> 'local_wcs_cache/wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits'
Saving the final (post-refit) wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits to local_wcs_cache/
'wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits' -> 'local_wcs_cache/wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits sigma_overall=0.327 worst_q_ratio=1.118
ref2=Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits sigma_overall=0.389 worst_q_ratio=1.093
new1=fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits sigma_overall=0.341 worst_q_ratio=1.156
new2=fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits sigma_overall=0.347 worst_q_ratio=1.098
reference average sigma_overall=0.358 worst_q_ratio=1.1055
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967_astrometric_residuals.png (4907 matched stars from wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968_astrometric_residuals.png (4908 matched stars from wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451_astrometric_residuals.png (3278 matched stars from wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452_astrometric_residuals.png (3287 matched stars from wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits'
Saving fully-calibrated image wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.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_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 00:38:41.40 +07:21:48.6: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 01:17:12.26 +02:00:46.5: 10.78 +/- 0.01 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 00:38:41.40 +07:21:48.6: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 01:17:12.26 +02:00:46.5: 10.77 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.77 +/- 0.00
Forced photometry filter REJECTED candidate at 01:17:12.26 +02:00:46.5: ref_mag=10.77 +/- 0.00 new_mean_mag=10.8414 delta=-0.07 (need > 0.90)
Adding exclusion_list_local.txt__out20206.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
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: 2s
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Considering the candidate 20190_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 20190_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
**** FOUND 00:25:34.96 +10:30:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20191_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
Preparing report for the candidate 20191_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
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Considering the candidate 20202_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
Preparing report for the candidate 20202_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
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Considering the candidate 20206_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
Preparing report for the candidate 20206_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
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Considering the candidate 20254_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 20254_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 8s
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 ####
00:38:41.40 +07:21:48.6
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
SExtractor catalog cache: saved Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits.cat to cache
SExtractor catalog cache: saved Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.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_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
Creating symlink local_wcs_cache/wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits exists and is non-empty
wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits exists and is non-empty
wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits exists and is non-empty
wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits (1st reference image)
verification OK: wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
Image size: 937.4'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:51:26.391 +05:59:58.81 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits (1st new image)
verification OK: wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits
Image size: 941.4'x626.8' 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: 00:51:36.078 +06:01:36.24 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:51:26.391 +05:59:58.81
Second-epoch image center 00:51:36.078 +06:01:36.24
Angular distance between the image centers 0.0484 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits (2nd new image)
verification OK: wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
Image size: 941.4'x626.8' 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: 00:51:33.584 +06:02:00.50 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:51:26.391 +05:59:58.81
Second-epoch image center 00:51:33.584 +06:02:00.50
Angular distance between the image centers 0.0451 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 00:51:36.078 +06:01:36.24
Second-epoch second image center 00:51:33.584 +06:02:00.50
Angular distance between the image centers 0.01234 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_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits &> /tmp/tmp.zZtY8o3AG1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits &> /tmp/tmp.CLA5vSKdlh
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits &> /tmp/tmp.UZk6Ax2h4J
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits &> /tmp/tmp.Waz1BbYMrO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.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_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits and wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.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_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits and wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits.wcscat
Found non-empty wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits and wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits.wcscat
The reference image (wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits) and catalog (wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits.wcscat) found
'wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits.wcscat' -> 'wcsmag.cat'
Read 29557 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 4.8579 to 20.7730 deg, Dec +0.6731 to +11.2752 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 4.8579 to 20.7730 deg, Dec 0.6731 to 11.2752 deg
Loaded 4462 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): 3659 out of 3874 total matches.
Matched with Tycho-2 3874 out of 29557 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.514200
a=0.000000 b=1.000000 c=22.514200
From vast_summary.log: estimated ref. image limiting mag.: -7.38
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.13
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.13
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 29557 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 4.8579 to 20.7730 deg, Dec +0.6731 to +11.2752 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 4.8579 to 20.7730 deg, Dec 0.6731 to 11.2752 deg
Loaded 4462 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): 3659 out of 3874 total matches.
Matched with Tycho-2 3874 out of 29557 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
Forced-photometry filter: calibrated wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits -> calib.txt_param_ref_wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits (aperture=5.1)
Read 30001 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 4.8801 to 20.7868 deg, Dec +0.6843 to +11.2881 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 4.8801 to 20.7868 deg, Dec 0.6843 to 11.2881 deg
Loaded 4460 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): 3639 out of 3862 total matches.
Matched with Tycho-2 3862 out of 30001 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits
Forced-photometry filter: calibrated wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits -> calib.txt_param_ref_wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits (aperture=5.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 37 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
2.1 pix Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits
1.9 pix fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits
1.9 pix fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
Limiting magnitude estimates:
15.1 mag. Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
15.1 mag. Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits
14.7 mag. fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits
14.7 mag. fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.1 (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.zZtY8o3AG1 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.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_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits' -> 'wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
WCS_IMAGE_NAME=wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
WCS-calibrated image found: wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
Checking if the catalog wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits.wcscat corresponding to the image wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits alredy exist and is non-empty...
Catalog wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits.wcscat corresponding to the image wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.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_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits
WCS catalog name: wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1115, bad_region=0, passed=29541
Got 29541 stars (including 28390 good ones) from the SExtractor catalog wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits.wcscat
util/solve_plate_with_UCAC5 got 29541 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4909 matched stars entering correct_measured_positions(), 4909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4909 matched stars entering correct_measured_positions(), 29541 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4908 matched stars entering correct_measured_positions(), 29541 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4908 matched stars entering correct_measured_positions(), 29541 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4908 stars left (next iteration limit 5399)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits N_match=4908 sigma_overall_arcsec=0.324 sigma_q1_arcsec=0.286 sigma_q2_arcsec=0.355 sigma_q3_arcsec=0.333 sigma_q4_arcsec=0.329 n_q1=1287 n_q2=1238 n_q3=1189 n_q4=1194 worst_quadrant_to_overall_ratio=1.094
The image catalog is written to wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits -region wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.CLA5vSKdlh (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.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_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits' -> 'wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits
WCS_IMAGE_NAME=wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits
WCS-calibrated image found: wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits
Checking if the catalog wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits.wcscat corresponding to the image wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits alredy exist and is non-empty...
Catalog wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits.wcscat corresponding to the image wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.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_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits
WCS catalog name: wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1096, bad_region=0, passed=29985
Got 29985 stars (including 28851 good ones) from the SExtractor catalog wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits.wcscat
util/solve_plate_with_UCAC5 got 29985 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4908 matched stars entering correct_measured_positions(), 4909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4908 matched stars entering correct_measured_positions(), 29985 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4908 matched stars entering correct_measured_positions(), 29985 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4908 matched stars entering correct_measured_positions(), 29985 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4908 stars left (next iteration limit 5398)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits N_match=4908 sigma_overall_arcsec=0.382 sigma_q1_arcsec=0.319 sigma_q2_arcsec=0.399 sigma_q3_arcsec=0.411 sigma_q4_arcsec=0.400 n_q1=1298 n_q2=1243 n_q3=1181 n_q4=1186 worst_quadrant_to_overall_ratio=1.076
The image catalog is written to wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits -region wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.UZk6Ax2h4J (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_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.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_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits
WCS_IMAGE_NAME=wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits
WCS-calibrated image found: wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits
Checking if the catalog wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits.wcscat corresponding to the image wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits.wcscat corresponding to the image wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.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_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits
WCS catalog name: wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.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=7, blended=642, bad_region=13, passed=23348
Got 23348 stars (including 22641 good ones) from the SExtractor catalog wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits.wcscat
util/solve_plate_with_UCAC5 got 23348 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 4917 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 4912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 23348 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 4918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 23348 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 23348 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4911 stars left (next iteration limit 5402)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4911 robust_rms=10.472 arcsec worst_quadrant_rms=11.027 arcsec
SIP_REFIT: SIP order 3 trial: matched=4911 robust_rms=0.509 arcsec worst_quadrant_rms=0.589 arcsec
SIP_REFIT: SIP order 5 trial: matched=4911 robust_rms=0.343 arcsec worst_quadrant_rms=0.412 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4911 robust_rms_before=1.001 arcsec robust_rms_before_corrected=0.347 arcsec robust_rms_after=0.343 arcsec worst_quadrant_rms_before=0.407 worst_quadrant_rms_after=0.412
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.407 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits N_match=4911 sigma_overall_arcsec=0.348 sigma_q1_arcsec=0.376 sigma_q2_arcsec=0.398 sigma_q3_arcsec=0.334 sigma_q4_arcsec=0.307 n_q1=1184 n_q2=1209 n_q3=1263 n_q4=1255 worst_quadrant_to_overall_ratio=1.144
The image catalog is written to wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits -region wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.Waz1BbYMrO (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_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.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_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
WCS_IMAGE_NAME=wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
WCS-calibrated image found: wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
Checking if the catalog wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits.wcscat corresponding to the image wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits.wcscat corresponding to the image wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.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_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
WCS catalog name: wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.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=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=651, bad_region=15, passed=23396
Got 23396 stars (including 22696 good ones) from the SExtractor catalog wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits.wcscat
util/solve_plate_with_UCAC5 got 23396 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 4919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4913 matched stars entering correct_measured_positions(), 4914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4913 matched stars entering correct_measured_positions(), 23396 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 4919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 23396 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 23396 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4911 stars left (next iteration limit 5404)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4911 robust_rms=10.487 arcsec worst_quadrant_rms=10.978 arcsec
SIP_REFIT: SIP order 3 trial: matched=4911 robust_rms=0.495 arcsec worst_quadrant_rms=0.579 arcsec
SIP_REFIT: SIP order 5 trial: matched=4911 robust_rms=0.340 arcsec worst_quadrant_rms=0.398 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4911 robust_rms_before=0.996 arcsec robust_rms_before_corrected=0.342 arcsec robust_rms_after=0.340 arcsec worst_quadrant_rms_before=0.397 worst_quadrant_rms_after=0.398
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.397 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits N_match=4911 sigma_overall_arcsec=0.351 sigma_q1_arcsec=0.377 sigma_q2_arcsec=0.406 sigma_q3_arcsec=0.339 sigma_q4_arcsec=0.300 n_q1=1178 n_q2=1195 n_q3=1271 n_q4=1267 worst_quadrant_to_overall_ratio=1.156
The image catalog is written to wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits -region wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.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_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-28-16_20.00sec_-0.00C_LIGHTs_0451.fits
Saving fully-calibrated image wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.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_2026-09-03_CI_Psc-05-Q1b1x1_061414_TTUQ1b1x1_3066251_ltqTp20I/wcs_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452.fits
Preparing the HTML report for the field Psc-05-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 00:48:07.43 +10:22:45.5: 13.18 +/- 0.03 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 00:50:57.16 +09:39:49.8: 13.04 +/- 0.03 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 01:15:45.12 +06:17:38.8: 14.17 +/- 0.09 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 01:11:45.69 +01:35:44.5: 13.30 +/- 0.04 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 01:16:50.11 +08:05:11.1: 12.87 +/- 0.03 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 00:32:45.20 +06:17:11.0: 13.50 +/- 0.05 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 00:22:57.70 +05:18:07.3: 12.96 +/- 0.03 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 01:13:57.39 +07:39:07.3: 14.06 +/- 0.08 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 01:19:55.65 +02:43:02.0: 13.55 +/- 0.06 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 01:18:12.07 +07:56:01.4: 12.90 +/- 0.03 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 01:16:50.11 +08:05:11.1: 12.82 +/- 0.03 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 00:48:07.43 +10:22:45.5: 13.20 +/- 0.03 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 01:19:55.65 +02:43:02.0: 13.38 +/- 0.05 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 01:13:57.39 +07:39:07.3: 14.08 +/- 0.09 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 01:15:45.12 +06:17:38.8: 14.14 +/- 0.09 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 00:22:57.70 +05:18:07.3: 13.01 +/- 0.04 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 00:50:57.16 +09:39:49.8: 13.05 +/- 0.03 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 00:32:45.20 +06:17:11.0: 13.64 +/- 0.05 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 01:11:45.69 +01:35:44.5: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Forced photometry reference-image weighted average: 14.07 +/- 0.06
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry reference-image weighted average: 13.45 +/- 0.04
Forced photometry reference-image weighted average: 14.16 +/- 0.06
Forced photometry filter REJECTED candidate at 01:16:50.11 +08:05:11.1: ref_mag=12.84 +/- 0.02 new_mean_mag=13.2417 delta=-0.40 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:48:07.43 +10:22:45.5: ref_mag=13.19 +/- 0.02 new_mean_mag=13.4195 delta=-0.23 (need > 0.90)
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Forced photometry filter REJECTED candidate at 01:19:55.65 +02:43:02.0: ref_mag=13.45 +/- 0.04 new_mean_mag=13.5104 delta=-0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:13:57.39 +07:39:07.3: ref_mag=14.07 +/- 0.06 new_mean_mag=13.9578 delta=0.11 (need > 0.90)
Forced photometry reference-image weighted average: 13.56 +/- 0.04
Forced photometry filter REJECTED candidate at 01:15:45.12 +06:17:38.8: ref_mag=14.16 +/- 0.06 new_mean_mag=14.1849 delta=-0.03 (need > 0.90)
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Forced photometry filter REJECTED candidate at 00:22:57.70 +05:18:07.3: ref_mag=12.98 +/- 0.02 new_mean_mag=13.1683 delta=-0.18 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:32:45.20 +06:17:11.0: ref_mag=13.56 +/- 0.04 new_mean_mag=13.9957 delta=-0.43 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:50:57.16 +09:39:49.8: ref_mag=13.04 +/- 0.02 new_mean_mag=13.6159 delta=-0.57 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:11:45.69 +01:35:44.5: ref_mag=13.30 +/- 0.03 new_mean_mag=13.5749 delta=-0.27 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 01:18:12.07 +07:56:01.4: 12.96 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.02
Forced photometry filter REJECTED candidate at 01:18:12.07 +07:56:01.4: ref_mag=12.93 +/- 0.02 new_mean_mag=13.3513 delta=-0.42 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 01:17:12.25 +02:00:46.6: 10.93 +/- 0.01 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 00:52:41.53 +06:11:34.5: 11.28 +/- 0.01 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 00:50:44.50 +04:07:05.4: 12.52 +/- 0.02 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 01:20:21.11 +02:48:03.3: 12.65 +/- 0.02 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 01:08:52.49 +09:13:40.9: 12.42 +/- 0.02 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 00:38:22.28 +08:36:54.9: 12.18 +/- 0.02 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 01:19:30.93 +07:28:42.3: 12.26 +/- 0.02 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 00:50:44.50 +04:07:05.4: 12.52 +/- 0.02 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 00:52:41.53 +06:11:34.5: 11.27 +/- 0.01 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 01:20:21.11 +02:48:03.3: 12.77 +/- 0.03 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 01:17:12.25 +02:00:46.6: 10.93 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Forced photometry reference-image weighted average: 11.28 +/- 0.00
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Forced photometry filter REJECTED candidate at 00:50:44.50 +04:07:05.4: ref_mag=12.52 +/- 0.01 new_mean_mag=12.8423 delta=-0.32 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 01:08:52.49 +09:13:40.9: 12.48 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.93 +/- 0.00
Forced photometry filter REJECTED candidate at 00:52:41.53 +06:11:34.5: ref_mag=11.28 +/- 0.00 new_mean_mag=11.7286 delta=-0.45 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:20:21.11 +02:48:03.3: ref_mag=12.71 +/- 0.02 new_mean_mag=12.7741 delta=-0.07 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:17:12.25 +02:00:46.6: ref_mag=10.93 +/- 0.00 new_mean_mag=10.8437 delta=0.08 (need > 0.90)
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Forced photometry filter REJECTED candidate at 01:08:52.49 +09:13:40.9: ref_mag=12.45 +/- 0.01 new_mean_mag=12.8127 delta=-0.37 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 00:38:22.28 +08:36:54.9: 12.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Forced photometry filter REJECTED candidate at 00:38:22.28 +08:36:54.9: ref_mag=12.19 +/- 0.01 new_mean_mag=12.2162 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 01:19:30.93 +07:28:42.3: 12.30 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.01
Forced photometry filter REJECTED candidate at 01:19:30.93 +07:28:42.3: ref_mag=12.28 +/- 0.01 new_mean_mag=12.3795 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 01:17:32.87 +08:55:05.7: 12.13 +/- 0.02 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 01:03:20.92 +00:46:37.0: 99.00 +/- 99.00 edge
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 00:37:34.74 +08:39:14.8: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 01:21:11.41 +02:35:15.4: 12.60 +/- 0.02 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 01:08:27.24 +05:10:42.4: 13.90 +/- 0.07 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 00:37:34.74 +08:39:14.8: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 01:03:20.92 +00:46:37.0: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 01:03:20.92 +00:46:37.0: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 01:17:32.87 +08:55:05.7: 12.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Forced photometry filter REJECTED candidate at 01:17:32.87 +08:55:05.7: ref_mag=12.14 +/- 0.01 new_mean_mag=12.6197 delta=-0.48 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 01:21:11.41 +02:35:15.4: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.02
Forced photometry filter REJECTED candidate at 01:21:11.41 +02:35:15.4: ref_mag=12.58 +/- 0.02 new_mean_mag=12.6218 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 00:24:04.16 +02:30:44.5: 15.46 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 00:35:22.79 +09:41:35.1: 13.44 +/- 0.05 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 01:08:27.24 +05:10:42.4: 13.90 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.05
Forced photometry filter REJECTED candidate at 01:08:27.24 +05:10:42.4: ref_mag=13.90 +/- 0.05 new_mean_mag=13.8685 delta=0.03 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 00:24:04.16 +02:30:44.5: 15.48 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 00:35:22.79 +09:41:35.1: 13.55 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Forced photometry filter REJECTED candidate at 00:35:22.79 +09:41:35.1: ref_mag=13.49 +/- 0.03 new_mean_mag=13.9781 delta=-0.49 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 00:42:23.50 +11:11:11.4: 13.91 +/- 0.07 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 00:28:02.87 +01:23:09.3: 15.30 +/- 0.30 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 01:20:47.60 +02:47:22.4: 14.49 +/- 0.14 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-39-23_20.00sec_5.00C_LIGHT_0967.fits at 01:18:29.43 +01:40:02.6: 14.59 +/- 0.15 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 00:42:23.50 +11:11:11.4: 14.10 +/- 0.09 detection
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 01:20:47.60 +02:47:22.4: 14.58 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.06
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 00:28:02.87 +01:23:09.3: 14.72 +/- 0.18 detection
Forced photometry filter REJECTED candidate at 00:42:23.50 +11:11:11.4: ref_mag=13.99 +/- 0.06 new_mean_mag=14.0006 delta=-0.01 (need > 0.90)
Forced photometry reference-image weighted average: 14.53 +/- 0.10
Forced photometry reference-image weighted average: 14.87 +/- 0.15
Forced photometry filter REJECTED candidate at 01:20:47.60 +02:47:22.4: ref_mag=14.53 +/- 0.10 new_mean_mag=14.2527 delta=0.28 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:28:02.87 +01:23:09.3: ref_mag=14.87 +/- 0.15 new_mean_mag=14.1454 delta=0.72 (need > 0.90)
Forced photometry on wcs_Psc-05-Q1b1x1_2026-07-21_04-40-22_20.00sec_5.00C_LIGHT_0968.fits at 01:18:29.43 +01:40:02.6: 14.76 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.66 +/- 0.11
Forced photometry filter REJECTED candidate at 01:18:29.43 +01:40:02.6: ref_mag=14.66 +/- 0.11 new_mean_mag=14.1971 delta=0.46 (need > 0.90)
Adding exclusion_list_local.txt__out33000.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33107.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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 32451_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 32451_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
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Considering the candidate 32452_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 32452_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
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Considering the candidate 32454_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 32454_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
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Considering the candidate 32458_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 32458_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
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Considering the candidate 32459_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 32459_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
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Considering the candidate 32460_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 32460_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
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Considering the candidate 32461_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 32461_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
**** FOUND 01:21:32.87 +09:14:09.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32462_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 32462_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
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Considering the candidate 32463_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 32463_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
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Considering the candidate 32464_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 32464_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
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Considering the candidate 32465_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 32465_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
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Considering the candidate 32466_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 32466_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
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Considering the candidate 32467_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 32467_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
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Considering the candidate 32468_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 32468_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
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Considering the candidate 32470_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 32470_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
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Considering the candidate 32471_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
Preparing report for the candidate 32471_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
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Considering the candidate 32482_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
Preparing report for the candidate 32482_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
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Considering the candidate 32486_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 32486_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
**** FOUND 00:38:41.40 +07:21:48.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 32530_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 32530_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
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Considering the candidate 32615_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
Preparing report for the candidate 32615_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
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Considering the candidate 32656_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 32656_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
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Considering the candidate 32674_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 32674_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
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Considering the candidate 32714_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 32714_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
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Considering the candidate 32724_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 32724_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
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Considering the candidate 32766_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 32766_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
**** FOUND 01:12:11.56 +00:50:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32866_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 32866_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
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Considering the candidate 33000_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
Preparing report for the candidate 33000_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
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Considering the candidate 33053_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 33053_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
**** FOUND 00:35:19.96 +04:06:10.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33054_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 33054_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
**** FOUND 00:50:58.23 +09:13:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33071_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 33071_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
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Considering the candidate 33107_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
Preparing report for the candidate 33107_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
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Considering the candidate 33132_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 33132_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
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Considering the candidate 33175_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 33175_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
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Considering the candidate 33208_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 33208_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
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Considering the candidate 33229_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 33229_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
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Considering the candidate 33243_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 33243_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
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Considering the candidate 03325_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452
The candidate 03325_fd_Psc-05-Q1b1x1_2026-09-03_05-29-15_20.00sec_-0.00C_LIGHTs_0452 did not pass the final checks
