This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 09 13.3649 2461296.8649 10.63 23:19:42.80 -00:20:38.4
79.71106 -55.32361 galactic Psc Second-epoch detections are separated by 0.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.236 Honoria 0 -0 0 10.7 -0 -0
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:19:42.80 -00:20:38.4: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:19:42.80 -00:20:38.4: 15.70 +/- 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,2461296.8649,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260913.3649 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.3649 2461296.8649 13.12 23:35:23.25 -00:23:46.7
85.45750 -57.62593 galactic Psc Second-epoch detections are separated by 0.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.570 Kythera 0 0 0 13.1 0 0
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:35:23.25 -00:23:46.7: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:35:23.25 -00:23:46.7: 15.64 +/- 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,2461296.8649,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260913.3649 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.3649 2461296.8649 13.12 23:30:35.51 -00:57:07.9
83.02620 -57.42081 galactic Psc Second-epoch detections are separated by 0.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.788 Hohensteina -0 0 0 13.4 -0 -0
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:30:35.51 -00:57:07.9: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:30:35.51 -00:57:07.9: 15.74 +/- 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,2461296.8649,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260913.3649 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.3649 2461296.8649 13.89 23:31:34.08 +00:51:11.0
85.23145 -56.05833 galactic Psc Second-epoch detections are separated by 0.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.673 Edda -0 0 0 13.9 -0 -0
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:31:34.08 +00:51:11.0: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:31:34.08 +00:51:11.0: 15.70 +/- 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,2461296.8649,13.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260913.3649 13.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.3649 2461296.8649 13.88 23:33:57.01 -05:54:20.1
78.48024 -61.89206 galactic Aqr Second-epoch detections are separated by 0.1" 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.981 Martina -0 0 0 14.1 0 0
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:33:57.01 -05:54:20.1: 15.27 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:33:57.01 -05:54:20.1: 15.23 +/- 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,2461296.8649,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260913.3649 13.88CV 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 13.3649 2461296.8649 14.14 23:24:34.35 +00:23:46.2
82.20533 -55.45189 galactic Psc Second-epoch detections are separated by 1.0" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1157 Arabia 0 0 0 14.0 -0 -0
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:24:34.35 +00:23:46.2: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:24:34.35 +00:23:46.2: 15.87 +/- 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,2461296.8649,14.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260913.3649 14.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461242.93564273 21.07.2026 10:27:09.532 /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
First image: 2461242.93564273 21.07.2026 10:27:09.532 /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
Last image: 2461296.86510193 13.09.2026 08:45:34.807 /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.46
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 7 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): 4761
Objects passed selection criteria: 4760
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 4623.75
Average stars matched: 4523.25 (97.8264 %)
Memory usage VmPeak: 232012 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 11 14:55:52 CDT 2026
VaST build number 1.0rc89-210-g97d43bca
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Sep 13 04:20:35 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: 2461242.93564273 21.07.2026 10:27:09.532 /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
First image: 2461242.93564273 21.07.2026 10:27:09.532 /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
Last image: 2461296.86510193 13.09.2026 08:45:34.807 /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 81
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.19
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: 19 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): 27011
Objects passed selection criteria: 26939
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 25507.2
Average stars matched: 24650.5 (96.6412 %)
Memory usage VmPeak: 252612 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 11 14:55:52 CDT 2026
VaST build number 1.0rc89-210-g97d43bca
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Sep 13 04:21:58 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
SExtractor catalog cache: saved Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.cat to cache
SExtractor catalog cache: saved Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.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: 2461296.86461498
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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits exists and is non-empty
wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits exists and is non-empty
wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits exists and is non-empty
wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits (1st reference image)
verification OK: wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
Image size: 937.5'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: 23:08:34.580 -02:00:27.91 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-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits (1st new image)
verification OK: wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits
Image size: 936.9'x624.0' 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: 23:08:55.508 -02:01:17.64 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:08:34.580 -02:00:27.91
Second-epoch image center 23:08:55.508 -02:01:17.64
Angular distance between the image centers 0.0882 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits (2nd new image)
verification OK: wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
Image size: 936.9'x624.0' 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: 23:08:53.255 -02:00:52.36 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:08:34.580 -02:00:27.91
Second-epoch image center 23:08:53.255 -02:00:52.36
Angular distance between the image centers 0.0781 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 23:08:55.508 -02:01:17.64
Second-epoch second image center 23:08:53.255 -02:00:52.36
Angular distance between the image centers 0.01172 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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits &> /tmp/tmp.KWe7kdoy5w
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits &> /tmp/tmp.BJHLOPa5oo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits &> /tmp/tmp.rSflJpKE0k
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits &> /tmp/tmp.ZjaCnloVlG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits and wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits and wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat
Found non-empty wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits and wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat
The reference image (wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits) and catalog (wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat) found
'wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat' -> 'wcsmag.cat'
Read 6415 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 339.2860 to 355.0261 deg, Dec -7.2671 to +3.2586 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 339.2860 to 355.0261 deg, Dec -7.2671 to 3.2586 deg
Loaded 4387 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): 3702 out of 3810 total matches.
Matched with Tycho-2 3810 out of 6415 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.655300
a=0.000000 b=1.000000 c=22.655300
From vast_summary.log: estimated ref. image limiting mag.: -7.46
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.20
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.20
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6415 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 339.2860 to 355.0261 deg, Dec -7.2671 to +3.2586 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 339.2860 to 355.0261 deg, Dec -7.2671 to 3.2586 deg
Loaded 4387 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): 3702 out of 3810 total matches.
Matched with Tycho-2 3810 out of 6415 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
Forced-photometry filter: calibrated wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits -> calib.txt_param_ref_wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits (aperture=6.3)
Read 6260 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 339.2725 to 355.0121 deg, Dec -7.2776 to +3.2517 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 339.2725 to 355.0121 deg, Dec -7.2776 to 3.2517 deg
Loaded 4385 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): 3695 out of 3795 total matches.
Matched with Tycho-2 3795 out of 6260 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
Forced-photometry filter: calibrated wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits -> calib.txt_param_ref_wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits (aperture=6.3)
____ 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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
2.2 pix Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
2.5 pix fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits
2.5 pix fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
Limiting magnitude estimates:
15.2 mag. Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
15.2 mag. Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
15.0 mag. fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits
15.0 mag. fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.KWe7kdoy5w (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits' -> 'wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
WCS_IMAGE_NAME=wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
WCS-calibrated image found: wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
Checking if the catalog wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat corresponding to the image wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits alredy exist and is non-empty...
Catalog wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat corresponding to the image wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
WCS catalog name: wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=388, bad_region=1637, passed=6415
Got 6415 stars (including 4478 good ones) from the SExtractor catalog wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat
util/solve_plate_with_UCAC5 got 6415 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4346 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4337 matched stars entering correct_measured_positions(), 4337 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4337 matched stars entering correct_measured_positions(), 5064 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4346 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4338 matched stars entering correct_measured_positions(), 5064 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4338 matched stars entering correct_measured_positions(), 5064 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4338 stars left (next iteration limit 4770)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits N_match=4338 sigma_overall_arcsec=0.314 sigma_q1_arcsec=0.310 sigma_q2_arcsec=0.326 sigma_q3_arcsec=0.299 sigma_q4_arcsec=0.295 n_q1=1429 n_q2=758 n_q3=1353 n_q4=798 worst_quadrant_to_overall_ratio=1.040
The image catalog is written to wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits -region wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.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.BJHLOPa5oo (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.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-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits' -> 'wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.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-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
WCS_IMAGE_NAME=wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
WCS-calibrated image found: wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
Checking if the catalog wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat corresponding to the image wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits alredy exist and is non-empty...
Catalog wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat corresponding to the image wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
WCS catalog name: wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=360, bad_region=1607, passed=6260
Got 6260 stars (including 4361 good ones) from the SExtractor catalog wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat
util/solve_plate_with_UCAC5 got 6260 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4238 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4230 matched stars entering correct_measured_positions(), 4230 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4230 matched stars entering correct_measured_positions(), 4940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4238 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4230 matched stars entering correct_measured_positions(), 4940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4230 matched stars entering correct_measured_positions(), 4940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4230 stars left (next iteration limit 4653)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits N_match=4230 sigma_overall_arcsec=0.379 sigma_q1_arcsec=0.359 sigma_q2_arcsec=0.403 sigma_q3_arcsec=0.382 sigma_q4_arcsec=0.346 n_q1=1416 n_q2=724 n_q3=1303 n_q4=787 worst_quadrant_to_overall_ratio=1.062
The image catalog is written to wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits -region wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.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.rSflJpKE0k (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_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.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_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits
WCS_IMAGE_NAME=wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits
WCS-calibrated image found: wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits
Checking if the catalog wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits.wcscat corresponding to the image wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits.wcscat corresponding to the image wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits
WCS catalog name: wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=369, bad_region=1212, passed=5820
Got 5820 stars (including 4392 good ones) from the SExtractor catalog wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits.wcscat
util/solve_plate_with_UCAC5 got 5820 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 413 to 468 (Dec -7.3 to 3.2)
Done reading UCAC5 zone files...
Matched 4269 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4265 matched stars entering correct_measured_positions(), 4265 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4265 matched stars entering correct_measured_positions(), 4842 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 413 to 468 (Dec -7.3 to 3.2)
Done reading UCAC5 zone files...
Matched 4269 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4265 matched stars entering correct_measured_positions(), 4842 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4265 matched stars entering correct_measured_positions(), 4842 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4265 stars left (next iteration limit 4691)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4265 robust_rms=6.659 arcsec worst_quadrant_rms=9.506 arcsec
SIP_REFIT: SIP order 3 trial: matched=4265 robust_rms=0.354 arcsec worst_quadrant_rms=0.376 arcsec
SIP_REFIT: SIP order 5 trial: matched=4265 robust_rms=0.322 arcsec worst_quadrant_rms=0.378 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=4265 robust_rms_before=0.943 arcsec robust_rms_before_corrected=0.313 arcsec robust_rms_after=0.354 arcsec worst_quadrant_rms_before=0.383 worst_quadrant_rms_after=0.376
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.383 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits N_match=4265 sigma_overall_arcsec=0.318 sigma_q1_arcsec=0.286 sigma_q2_arcsec=0.368 sigma_q3_arcsec=0.295 sigma_q4_arcsec=0.379 n_q1=1454 n_q2=749 n_q3=1316 n_q4=746 worst_quadrant_to_overall_ratio=1.194
The image catalog is written to wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits -region wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.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.ZjaCnloVlG (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_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.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_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
WCS_IMAGE_NAME=wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
WCS-calibrated image found: wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
Checking if the catalog wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits.wcscat corresponding to the image wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits.wcscat corresponding to the image wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
WCS catalog name: wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=440, bad_region=1227, passed=5813
Got 5813 stars (including 4356 good ones) from the SExtractor catalog wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits.wcscat
util/solve_plate_with_UCAC5 got 5813 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 413 to 468 (Dec -7.3 to 3.2)
Done reading UCAC5 zone files...
Matched 4234 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4231 matched stars entering correct_measured_positions(), 4231 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4231 matched stars entering correct_measured_positions(), 4817 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 413 to 468 (Dec -7.3 to 3.2)
Done reading UCAC5 zone files...
Matched 4234 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4230 matched stars entering correct_measured_positions(), 4817 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4230 matched stars entering correct_measured_positions(), 4817 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4230 stars left (next iteration limit 4654)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4230 robust_rms=6.575 arcsec worst_quadrant_rms=9.064 arcsec
SIP_REFIT: SIP order 3 trial: matched=4230 robust_rms=0.362 arcsec worst_quadrant_rms=0.387 arcsec
SIP_REFIT: SIP order 5 trial: matched=4230 robust_rms=0.329 arcsec worst_quadrant_rms=0.390 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=4230 robust_rms_before=0.949 arcsec robust_rms_before_corrected=0.318 arcsec robust_rms_after=0.362 arcsec worst_quadrant_rms_before=0.385 worst_quadrant_rms_after=0.387
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.385 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits N_match=4230 sigma_overall_arcsec=0.316 sigma_q1_arcsec=0.277 sigma_q2_arcsec=0.394 sigma_q3_arcsec=0.291 sigma_q4_arcsec=0.375 n_q1=1443 n_q2=728 n_q3=1305 n_q4=754 worst_quadrant_to_overall_ratio=1.245
The image catalog is written to wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits -region wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits to local_wcs_cache/
'wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits' -> 'local_wcs_cache/wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits'
Saving the final (post-refit) wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits to local_wcs_cache/
'wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits' -> 'local_wcs_cache/wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits'
Saving the final (post-refit) wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits to local_wcs_cache/
'wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits' -> 'local_wcs_cache/wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits'
Saving the final (post-refit) wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits to local_wcs_cache/
'wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits' -> 'local_wcs_cache/wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits sigma_overall=0.314 worst_q_ratio=1.040
ref2=Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits sigma_overall=0.379 worst_q_ratio=1.062
new1=fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits sigma_overall=0.318 worst_q_ratio=1.194
new2=fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits sigma_overall=0.316 worst_q_ratio=1.245
reference average sigma_overall=0.3465 worst_q_ratio=1.051
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017_astrometric_residuals.png (4338 matched stars from wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018_astrometric_residuals.png (4230 matched stars from wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212_astrometric_residuals.png (4265 matched stars from wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213_astrometric_residuals.png (4230 matched stars from wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits'
Saving fully-calibrated image wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits'
Preparing the HTML report for the field Psc-09-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:09:54.78 -00:33:18.1: 12.18 +/- 0.01 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:19:42.80 -00:20:38.4: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:07:13.50 -01:29:21.4: 12.06 +/- 0.01 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:21:26.73 -03:04:03.0: 11.57 +/- 0.01 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:01:58.98 +00:24:25.0: 12.00 +/- 0.01 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:09:54.78 -00:33:18.1: 12.22 +/- 0.01 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:07:13.50 -01:29:21.4: 12.07 +/- 0.01 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:01:58.98 +00:24:25.0: 11.99 +/- 0.01 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:19:42.80 -00:20:38.4: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:21:26.73 -03:04:03.0: 11.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.01
Forced photometry reference-image weighted average: 12.06 +/- 0.01
Forced photometry reference-image weighted average: 11.99 +/- 0.01
Forced photometry filter REJECTED candidate at 23:09:54.78 -00:33:18.1: ref_mag=12.20 +/- 0.01 new_mean_mag=12.1763 delta=0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:07:13.50 -01:29:21.4: ref_mag=12.06 +/- 0.01 new_mean_mag=12.0934 delta=-0.03 (need > 0.90)
Forced photometry reference-image weighted average: 11.56 +/- 0.01
Forced photometry filter REJECTED candidate at 23:01:58.98 +00:24:25.0: ref_mag=11.99 +/- 0.01 new_mean_mag=12.0235 delta=-0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:21:26.73 -03:04:03.0: ref_mag=11.56 +/- 0.01 new_mean_mag=11.7168 delta=-0.15 (need > 0.90)
Adding exclusion_list_local.txt__out20228.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
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 20228_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 20228_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 20238_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 20238_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 20241_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 20241_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20245_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 20245_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20248_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 20248_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 10s
Prepared the HTML report for the field Psc-09-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
23:19:42.80 -00:20:38.4
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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
SExtractor catalog cache: saved Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.cat to cache
SExtractor catalog cache: saved Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
Creating symlink local_wcs_cache/wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits exists and is non-empty
wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits exists and is non-empty
wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits exists and is non-empty
wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits (1st reference image)
verification OK: wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
Image size: 937.5'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: 23:08:34.580 -02:00:27.91 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-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits (1st new image)
verification OK: wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits
Image size: 936.9'x624.0' 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: 23:08:55.508 -02:01:17.64 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:08:34.580 -02:00:27.91
Second-epoch image center 23:08:55.508 -02:01:17.64
Angular distance between the image centers 0.0882 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits (2nd new image)
verification OK: wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
Image size: 936.9'x624.0' 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: 23:08:53.255 -02:00:52.36 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:08:34.580 -02:00:27.91
Second-epoch image center 23:08:53.255 -02:00:52.36
Angular distance between the image centers 0.0781 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 23:08:55.508 -02:01:17.64
Second-epoch second image center 23:08:53.255 -02:00:52.36
Angular distance between the image centers 0.01172 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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits &> /tmp/tmp.RdUHX38xax
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits &> /tmp/tmp.LVg9UO8xOd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits &> /tmp/tmp.msoOVTHGrr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits &> /tmp/tmp.wSPmSlOV0X
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits and wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits and wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat
Found non-empty wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits and wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat
The reference image (wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits) and catalog (wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat) found
'wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat' -> 'wcsmag.cat'
Read 35879 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 339.2853 to 355.0336 deg, Dec -7.2742 to +3.2602 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 339.2853 to 355.0336 deg, Dec -7.2742 to 3.2602 deg
Loaded 4394 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): 3591 out of 3893 total matches.
Matched with Tycho-2 3893 out of 35879 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.537600
a=0.000000 b=1.000000 c=22.537600
From vast_summary.log: estimated ref. image limiting mag.: -7.19
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.35
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.35
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 35879 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 339.2853 to 355.0336 deg, Dec -7.2742 to +3.2602 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 339.2853 to 355.0336 deg, Dec -7.2742 to 3.2602 deg
Loaded 4394 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): 3591 out of 3893 total matches.
Matched with Tycho-2 3893 out of 35879 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
Forced-photometry filter: calibrated wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits -> calib.txt_param_ref_wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits (aperture=4.9)
Read 36137 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 339.2724 to 355.0227 deg, Dec -7.2779 to +3.2557 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 339.2724 to 355.0227 deg, Dec -7.2779 to 3.2557 deg
Loaded 4393 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): 3594 out of 3890 total matches.
Matched with Tycho-2 3890 out of 36137 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
Forced-photometry filter: calibrated wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits -> calib.txt_param_ref_wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 54 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
2.1 pix Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
2.5 pix fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits
2.4 pix fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
Limiting magnitude estimates:
15.4 mag. Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
15.4 mag. Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
15.1 mag. fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits
15.1 mag. fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 14.3 (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.RdUHX38xax (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits' -> 'wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
WCS_IMAGE_NAME=wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
WCS-calibrated image found: wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
Checking if the catalog wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat corresponding to the image wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits alredy exist and is non-empty...
Catalog wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat corresponding to the image wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
WCS catalog name: wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=1717, bad_region=7702, passed=35853
Got 35853 stars (including 26731 good ones) from the SExtractor catalog wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat
util/solve_plate_with_UCAC5 got 35853 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4863 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 4852 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 29872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4863 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 29872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 29872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4852 stars left (next iteration limit 5337)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits N_match=4852 sigma_overall_arcsec=0.314 sigma_q1_arcsec=0.319 sigma_q2_arcsec=0.329 sigma_q3_arcsec=0.303 sigma_q4_arcsec=0.299 n_q1=1558 n_q2=904 n_q3=1485 n_q4=905 worst_quadrant_to_overall_ratio=1.048
The image catalog is written to wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits -region wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.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.LVg9UO8xOd (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.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-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits' -> 'wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.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-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
WCS_IMAGE_NAME=wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
WCS-calibrated image found: wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
Checking if the catalog wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat corresponding to the image wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits alredy exist and is non-empty...
Catalog wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat corresponding to the image wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
WCS catalog name: wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=8, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=1465, bad_region=7825, passed=36110
Got 36110 stars (including 27137 good ones) from the SExtractor catalog wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat
util/solve_plate_with_UCAC5 got 36110 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4861 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4854 matched stars entering correct_measured_positions(), 4854 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4854 matched stars entering correct_measured_positions(), 30009 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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4861 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4854 matched stars entering correct_measured_positions(), 30009 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4854 matched stars entering correct_measured_positions(), 30009 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4854 stars left (next iteration limit 5339)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.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-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits N_match=4854 sigma_overall_arcsec=0.372 sigma_q1_arcsec=0.361 sigma_q2_arcsec=0.408 sigma_q3_arcsec=0.377 sigma_q4_arcsec=0.355 n_q1=1577 n_q2=898 n_q3=1478 n_q4=901 worst_quadrant_to_overall_ratio=1.095
The image catalog is written to wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits -region wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.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.msoOVTHGrr (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_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.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_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits
WCS_IMAGE_NAME=wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits
WCS-calibrated image found: wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits
Checking if the catalog wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits.wcscat corresponding to the image wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits.wcscat corresponding to the image wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits
WCS catalog name: wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1850, bad_region=4667, passed=27773
Got 27773 stars (including 22323 good ones) from the SExtractor catalog wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits.wcscat
util/solve_plate_with_UCAC5 got 27773 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 413 to 468 (Dec -7.3 to 3.2)
Done reading UCAC5 zone files...
Matched 4853 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4850 matched stars entering correct_measured_positions(), 4850 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4850 matched stars entering correct_measured_positions(), 24129 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 413 to 468 (Dec -7.3 to 3.2)
Done reading UCAC5 zone files...
Matched 4853 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4851 matched stars entering correct_measured_positions(), 24129 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4851 matched stars entering correct_measured_positions(), 24130 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4851 stars left (next iteration limit 5335)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.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=4851 robust_rms=6.211 arcsec worst_quadrant_rms=10.202 arcsec
SIP_REFIT: SIP order 3 trial: matched=4851 robust_rms=0.359 arcsec worst_quadrant_rms=0.376 arcsec
SIP_REFIT: SIP order 5 trial: matched=4851 robust_rms=0.326 arcsec worst_quadrant_rms=0.374 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=4851 robust_rms_before=0.953 arcsec robust_rms_before_corrected=0.319 arcsec robust_rms_after=0.359 arcsec worst_quadrant_rms_before=0.367 worst_quadrant_rms_after=0.376
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.367 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits N_match=4851 sigma_overall_arcsec=0.322 sigma_q1_arcsec=0.300 sigma_q2_arcsec=0.373 sigma_q3_arcsec=0.303 sigma_q4_arcsec=0.365 n_q1=1679 n_q2=800 n_q3=1546 n_q4=826 worst_quadrant_to_overall_ratio=1.158
The image catalog is written to wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits -region wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.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.wSPmSlOV0X (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_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.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_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
WCS_IMAGE_NAME=wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
WCS-calibrated image found: wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
Checking if the catalog wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits.wcscat corresponding to the image wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits.wcscat corresponding to the image wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
WCS catalog name: wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1985, bad_region=4710, passed=28096
Got 28096 stars (including 22569 good ones) from the SExtractor catalog wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits.wcscat
util/solve_plate_with_UCAC5 got 28096 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4853 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4847 matched stars entering correct_measured_positions(), 4847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4847 matched stars entering correct_measured_positions(), 24380 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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4853 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4847 matched stars entering correct_measured_positions(), 24380 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4847 matched stars entering correct_measured_positions(), 24380 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4847 stars left (next iteration limit 5331)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.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=4847 robust_rms=6.173 arcsec worst_quadrant_rms=10.094 arcsec
SIP_REFIT: SIP order 3 trial: matched=4847 robust_rms=0.363 arcsec worst_quadrant_rms=0.380 arcsec
SIP_REFIT: SIP order 5 trial: matched=4847 robust_rms=0.331 arcsec worst_quadrant_rms=0.382 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=4847 robust_rms_before=0.951 arcsec robust_rms_before_corrected=0.314 arcsec robust_rms_after=0.363 arcsec worst_quadrant_rms_before=0.372 worst_quadrant_rms_after=0.380
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-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits N_match=4847 sigma_overall_arcsec=0.321 sigma_q1_arcsec=0.285 sigma_q2_arcsec=0.381 sigma_q3_arcsec=0.308 sigma_q4_arcsec=0.374 n_q1=1682 n_q2=798 n_q3=1550 n_q4=817 worst_quadrant_to_overall_ratio=1.185
The image catalog is written to wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits -region wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.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-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.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_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-44-52_20.00sec_-0.00C_LIGHT_0212.fits
Saving fully-calibrated image wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.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_2026-09-13_CI_Psc-09-Q2b1x1_041108_TTUQ2b1x1_1078638_kqyIjELe/wcs_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213.fits
Preparing the HTML report for the field Psc-09-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:31:34.08 +00:51:11.0: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:30:35.51 -00:57:07.9: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:24:17.15 -06:14:03.9: 13.25 +/- 0.04 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:24:50.86 +00:27:20.4: 13.64 +/- 0.05 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:35:23.25 -00:23:46.7: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:28:50.51 -05:22:21.7: 13.58 +/- 0.06 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:26:38.15 -05:12:46.6: 13.03 +/- 0.04 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:24:26.38 +00:13:25.6: 15.11 +/- 0.19 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:29:32.37 -01:46:37.8: 12.72 +/- 0.03 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:33:57.01 -05:54:20.1: 15.27 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:24:50.86 +00:27:20.4: 13.61 +/- 0.05 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:24:17.15 -06:14:03.9: 13.27 +/- 0.04 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:28:50.51 -05:22:21.7: 13.56 +/- 0.07 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:30:35.51 -00:57:07.9: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:35:23.25 -00:23:46.7: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:31:34.08 +00:51:11.0: 15.70 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Forced photometry reference-image weighted average: 13.26 +/- 0.03
Forced photometry filter REJECTED candidate at 23:24:50.86 +00:27:20.4: ref_mag=13.62 +/- 0.03 new_mean_mag=14.0054 delta=-0.38 (need > 0.90)
Forced photometry reference-image weighted average: 13.57 +/- 0.05
Forced photometry filter REJECTED candidate at 23:24:17.15 -06:14:03.9: ref_mag=13.26 +/- 0.03 new_mean_mag=13.4281 delta=-0.17 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:24:26.38 +00:13:25.6: 14.84 +/- 0.15 detection
Forced photometry filter REJECTED candidate at 23:28:50.51 -05:22:21.7: ref_mag=13.57 +/- 0.05 new_mean_mag=13.8029 delta=-0.23 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:29:32.37 -01:46:37.8: 12.75 +/- 0.03 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:26:38.15 -05:12:46.6: 13.07 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.02
Forced photometry reference-image weighted average: 13.05 +/- 0.03
Forced photometry reference-image weighted average: 14.95 +/- 0.12
Forced photometry filter REJECTED candidate at 23:29:32.37 -01:46:37.8: ref_mag=12.73 +/- 0.02 new_mean_mag=12.7281 delta=0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:26:38.15 -05:12:46.6: ref_mag=13.05 +/- 0.03 new_mean_mag=13.0348 delta=0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:24:26.38 +00:13:25.6: ref_mag=14.95 +/- 0.12 new_mean_mag=14.7219 delta=0.23 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:33:57.01 -05:54:20.1: 15.23 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:32:06.30 +00:02:55.9: 13.94 +/- 0.07 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:29:29.36 -00:58:11.1: 14.30 +/- 0.10 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:24:34.35 +00:23:46.2: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:21:22.45 -03:24:14.7: 14.21 +/- 0.09 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:35:43.63 -02:57:42.9: 14.74 +/- 0.17 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:15:39.22 -02:16:31.8: 14.19 +/- 0.08 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:32:06.30 +00:02:55.9: 13.95 +/- 0.07 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:29:29.36 -00:58:11.1: 14.11 +/- 0.08 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:24:34.35 +00:23:46.2: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:21:22.45 -03:24:14.7: 14.11 +/- 0.08 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:35:43.63 -02:57:42.9: 14.65 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.05
Forced photometry reference-image weighted average: 14.19 +/- 0.06
Forced photometry filter REJECTED candidate at 23:32:06.30 +00:02:55.9: ref_mag=13.94 +/- 0.05 new_mean_mag=14.0897 delta=-0.15 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:29:29.36 -00:58:11.1: ref_mag=14.19 +/- 0.06 new_mean_mag=14.1496 delta=0.04 (need > 0.90)
Forced photometry reference-image weighted average: 14.15 +/- 0.06
Forced photometry filter REJECTED candidate at 23:21:22.45 -03:24:14.7: ref_mag=14.15 +/- 0.06 new_mean_mag=14.0276 delta=0.12 (need > 0.90)
Forced photometry reference-image weighted average: 14.69 +/- 0.12
Forced photometry filter REJECTED candidate at 23:35:43.63 -02:57:42.9: ref_mag=14.69 +/- 0.12 new_mean_mag=14.4228 delta=0.27 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:15:39.22 -02:16:31.8: 14.23 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.21 +/- 0.06
Forced photometry filter REJECTED candidate at 23:15:39.22 -02:16:31.8: ref_mag=14.21 +/- 0.06 new_mean_mag=14.3087 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:31:47.99 -01:06:20.3: 14.60 +/- 0.15 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:31:32.90 -06:01:42.4: 15.00 +/- 0.21 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:33:16.15 -02:10:46.6: 14.87 +/- 0.18 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:33:28.67 -01:59:00.1: 14.71 +/- 0.16 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:35:27.91 -03:45:52.7: 14.77 +/- 0.17 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:31:47.99 -01:06:20.3: 14.63 +/- 0.16 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:33:16.15 -02:10:46.6: 14.52 +/- 0.13 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:31:32.90 -06:01:42.4: 14.88 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.61 +/- 0.11
Forced photometry reference-image weighted average: 14.64 +/- 0.10
Forced photometry filter REJECTED candidate at 23:31:47.99 -01:06:20.3: ref_mag=14.61 +/- 0.11 new_mean_mag=14.5862 delta=0.03 (need > 0.90)
Forced photometry reference-image weighted average: 14.94 +/- 0.15
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:33:28.67 -01:59:00.1: 14.76 +/- 0.16 detection
Forced photometry filter REJECTED candidate at 23:33:16.15 -02:10:46.6: ref_mag=14.64 +/- 0.10 new_mean_mag=14.5982 delta=0.04 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:31:32.90 -06:01:42.4: ref_mag=14.94 +/- 0.15 new_mean_mag=14.5397 delta=0.40 (need > 0.90)
Forced photometry reference-image weighted average: 14.74 +/- 0.11
Forced photometry filter REJECTED candidate at 23:33:28.67 -01:59:00.1: ref_mag=14.74 +/- 0.11 new_mean_mag=14.5245 delta=0.21 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:35:27.91 -03:45:52.7: 14.93 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.84 +/- 0.13
Forced photometry filter REJECTED candidate at 23:35:27.91 -03:45:52.7: ref_mag=14.84 +/- 0.13 new_mean_mag=14.5464 delta=0.29 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:36:20.67 -03:27:51.6: 14.42 +/- 0.13 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:21:23.06 -03:05:04.6: 14.54 +/- 0.13 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:27:07.15 -01:17:42.4: 14.25 +/- 0.10 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:35:35.01 -01:39:03.0: 15.18 +/- 0.24 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:34:21.61 -01:06:22.3: 14.83 +/- 0.17 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:36:20.67 -03:27:51.6: 14.76 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.52 +/- 0.11
Forced photometry filter REJECTED candidate at 23:36:20.67 -03:27:51.6: ref_mag=14.52 +/- 0.11 new_mean_mag=14.5162 delta=0.01 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:21:23.06 -03:05:04.6: 14.38 +/- 0.11 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:27:07.15 -01:17:42.4: 14.26 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.45 +/- 0.08
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:35:35.01 -01:39:03.0: 15.02 +/- 0.21 detection
Forced photometry filter REJECTED candidate at 23:21:23.06 -03:05:04.6: ref_mag=14.45 +/- 0.08 new_mean_mag=14.5327 delta=-0.08 (need > 0.90)
Forced photometry reference-image weighted average: 14.25 +/- 0.07
Forced photometry reference-image weighted average: 15.09 +/- 0.16
Forced photometry filter REJECTED candidate at 23:27:07.15 -01:17:42.4: ref_mag=14.25 +/- 0.07 new_mean_mag=14.3929 delta=-0.14 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:35:35.01 -01:39:03.0: ref_mag=15.09 +/- 0.16 new_mean_mag=14.6454 delta=0.44 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:34:21.61 -01:06:22.3: 14.81 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.82 +/- 0.12
Forced photometry filter REJECTED candidate at 23:34:21.61 -01:06:22.3: ref_mag=14.82 +/- 0.12 new_mean_mag=14.5514 delta=0.26 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:34:12.04 -03:17:11.0: 14.82 +/- 0.17 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:34:26.99 -04:33:17.5: 14.95 +/- 0.21 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:29:35.28 -00:20:31.8: 14.86 +/- 0.16 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:34:36.79 -01:58:54.8: 14.63 +/- 0.14 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:24:36.25 -04:04:57.6: 15.00 +/- 0.19 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:34:12.04 -03:17:11.0: 15.04 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.91 +/- 0.13
Forced photometry filter REJECTED candidate at 23:34:12.04 -03:17:11.0: ref_mag=14.91 +/- 0.13 new_mean_mag=14.6631 delta=0.24 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:34:26.99 -04:33:17.5: 15.19 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.04 +/- 0.16
Forced photometry filter REJECTED candidate at 23:34:26.99 -04:33:17.5: ref_mag=15.04 +/- 0.16 new_mean_mag=14.6873 delta=0.36 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:29:35.28 -00:20:31.8: 15.23 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.99 +/- 0.13
Forced photometry filter REJECTED candidate at 23:29:35.28 -00:20:31.8: ref_mag=14.99 +/- 0.13 new_mean_mag=14.6401 delta=0.35 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:24:36.25 -04:04:57.6: 14.97 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.98 +/- 0.13
Forced photometry filter REJECTED candidate at 23:24:36.25 -04:04:57.6: ref_mag=14.98 +/- 0.13 new_mean_mag=14.6203 delta=0.36 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:34:36.79 -01:58:54.8: 14.76 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.69 +/- 0.11
Forced photometry filter REJECTED candidate at 23:34:36.79 -01:58:54.8: ref_mag=14.69 +/- 0.11 new_mean_mag=14.6445 delta=0.04 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:26:27.24 -04:57:55.1: 14.97 +/- 0.19 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:34:10.04 -02:20:22.2: 14.92 +/- 0.19 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:31:49.23 -04:49:15.2: 14.78 +/- 0.17 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:28:29.54 -04:53:30.6: 15.10 +/- 0.23 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:34:24.15 -05:55:29.9: 14.44 +/- 0.14 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:26:27.24 -04:57:55.1: 14.68 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.79 +/- 0.12
Forced photometry filter REJECTED candidate at 23:26:27.24 -04:57:55.1: ref_mag=14.79 +/- 0.12 new_mean_mag=14.4823 delta=0.31 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:34:10.04 -02:20:22.2: 15.04 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.98 +/- 0.14
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:31:49.23 -04:49:15.2: 14.87 +/- 0.18 detection
Forced photometry filter REJECTED candidate at 23:34:10.04 -02:20:22.2: ref_mag=14.98 +/- 0.14 new_mean_mag=14.4399 delta=0.54 (need > 0.90)
Forced photometry reference-image weighted average: 14.82 +/- 0.12
Forced photometry filter REJECTED candidate at 23:31:49.23 -04:49:15.2: ref_mag=14.82 +/- 0.12 new_mean_mag=14.7121 delta=0.11 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:28:29.54 -04:53:30.6: 14.67 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.80 +/- 0.12
Forced photometry filter REJECTED candidate at 23:28:29.54 -04:53:30.6: ref_mag=14.80 +/- 0.12 new_mean_mag=14.7278 delta=0.07 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:34:24.15 -05:55:29.9: 14.88 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.58 +/- 0.12
Forced photometry filter REJECTED candidate at 23:34:24.15 -05:55:29.9: ref_mag=14.58 +/- 0.12 new_mean_mag=14.4808 delta=0.10 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:31:17.89 -00:43:19.0: 14.76 +/- 0.15 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:35:18.02 -02:26:37.8: 14.81 +/- 0.18 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:30:35.20 -03:11:23.9: 15.29 +/- 0.26 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:28:45.62 -00:31:11.7: 14.56 +/- 0.13 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:35:25.60 +01:03:32.7: 14.69 +/- 0.15 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:31:17.89 -00:43:19.0: 14.79 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.77 +/- 0.11
Forced photometry filter REJECTED candidate at 23:31:17.89 -00:43:19.0: ref_mag=14.77 +/- 0.11 new_mean_mag=14.7406 delta=0.03 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:35:18.02 -02:26:37.8: 14.87 +/- 0.19 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:30:35.20 -03:11:23.9: 15.05 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.84 +/- 0.13
Forced photometry filter REJECTED candidate at 23:35:18.02 -02:26:37.8: ref_mag=14.84 +/- 0.13 new_mean_mag=14.8462 delta=-0.01 (need > 0.90)
Forced photometry reference-image weighted average: 15.14 +/- 0.16
Forced photometry filter REJECTED candidate at 23:30:35.20 -03:11:23.9: ref_mag=15.14 +/- 0.16 new_mean_mag=14.8147 delta=0.32 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:28:45.62 -00:31:11.7: 14.61 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.59 +/- 0.09
Forced photometry filter REJECTED candidate at 23:28:45.62 -00:31:11.7: ref_mag=14.59 +/- 0.09 new_mean_mag=14.6181 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:35:25.60 +01:03:32.7: 15.00 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.80 +/- 0.12
Forced photometry filter REJECTED candidate at 23:35:25.60 +01:03:32.7: ref_mag=14.80 +/- 0.12 new_mean_mag=14.6767 delta=0.13 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:35:55.94 +00:18:37.6: 14.64 +/- 0.15 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:30:36.51 -04:15:45.4: 15.27 +/- 0.25 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:34:27.49 +00:45:45.7: 14.93 +/- 0.18 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:32:51.73 -03:17:39.9: 15.42 +/- 0.30 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:31:33.67 -00:26:35.4: 15.00 +/- 0.19 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:35:55.94 +00:18:37.6: 14.81 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.71 +/- 0.11
Forced photometry filter REJECTED candidate at 23:35:55.94 +00:18:37.6: ref_mag=14.71 +/- 0.11 new_mean_mag=14.8002 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:30:36.51 -04:15:45.4: 15.08 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.16 +/- 0.16
Forced photometry filter REJECTED candidate at 23:30:36.51 -04:15:45.4: ref_mag=15.16 +/- 0.16 new_mean_mag=14.7483 delta=0.41 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:34:27.49 +00:45:45.7: 15.27 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.03 +/- 0.15
Forced photometry filter REJECTED candidate at 23:34:27.49 +00:45:45.7: ref_mag=15.03 +/- 0.15 new_mean_mag=14.8666 delta=0.17 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:32:51.73 -03:17:39.9: 15.51 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.46 +/- 0.22
Forced photometry filter REJECTED candidate at 23:32:51.73 -03:17:39.9: ref_mag=15.46 +/- 0.22 new_mean_mag=14.6698 delta=0.79 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:31:33.67 -00:26:35.4: 15.42 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.14 +/- 0.15
Forced photometry filter REJECTED candidate at 23:31:33.67 -00:26:35.4: ref_mag=15.14 +/- 0.15 new_mean_mag=14.8284 delta=0.31 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:26:12.62 +00:06:37.6: 14.99 +/- 0.18 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:25:44.83 +01:00:50.2: 14.75 +/- 0.14 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:28:06.22 -00:53:01.4: 15.06 +/- 0.19 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:30:58.51 -06:11:29.8: 15.05 +/- 0.23 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:19:31.71 +00:49:17.9: 15.60 +/- 0.29 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:26:12.62 +00:06:37.6: 14.77 +/- 0.14 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:25:44.83 +01:00:50.2: 14.71 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.85 +/- 0.11
Forced photometry reference-image weighted average: 14.73 +/- 0.10
Forced photometry filter REJECTED candidate at 23:26:12.62 +00:06:37.6: ref_mag=14.85 +/- 0.11 new_mean_mag=14.8391 delta=0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:25:44.83 +01:00:50.2: ref_mag=14.73 +/- 0.10 new_mean_mag=14.5225 delta=0.21 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:28:06.22 -00:53:01.4: 15.12 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.09 +/- 0.14
Forced photometry filter REJECTED candidate at 23:28:06.22 -00:53:01.4: ref_mag=15.09 +/- 0.14 new_mean_mag=14.7566 delta=0.33 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:30:58.51 -06:11:29.8: 14.74 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.84 +/- 0.13
Forced photometry filter REJECTED candidate at 23:30:58.51 -06:11:29.8: ref_mag=14.84 +/- 0.13 new_mean_mag=14.8129 delta=0.03 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:19:31.71 +00:49:17.9: 15.34 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.44 +/- 0.17
Forced photometry filter REJECTED candidate at 23:19:31.71 +00:49:17.9: ref_mag=15.44 +/- 0.17 new_mean_mag=14.8816 delta=0.55 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:20:35.73 -03:11:42.4: 14.79 +/- 0.15 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:20:35.73 -03:11:42.4: 14.96 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.86 +/- 0.11
Forced photometry filter REJECTED candidate at 23:20:35.73 -03:11:42.4: ref_mag=14.86 +/- 0.11 new_mean_mag=14.8801 delta=-0.02 (need > 0.90)
Adding exclusion_list_local.txt__out52564.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52565.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52615.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52663.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
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 52493_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52493_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52498_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52498_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52516_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52516_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
**** FOUND 23:19:42.80 -00:20:38.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52554_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52554_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52564_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 52564_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 52565_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 52565_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 52569_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52569_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52589_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52589_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52611_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52611_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52615_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 52615_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 52627_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 52627_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 52633_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52633_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52642_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52642_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52646_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52646_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52663_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
Preparing report for the candidate 52663_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
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Considering the candidate 52665_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52665_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52678_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52678_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52682_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52682_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52685_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52685_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52687_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52687_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52688_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52688_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52691_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52691_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52695_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52695_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52696_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52696_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52697_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52697_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52704_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52704_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52705_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52705_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52706_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52706_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52708_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52708_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52718_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52718_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52719_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52719_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52726_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52726_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52728_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52728_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52731_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52731_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52737_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52737_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52746_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52746_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52747_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52747_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52749_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52749_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52752_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52752_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52753_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52753_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52760_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52760_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52761_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52761_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52763_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52763_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52764_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52764_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52767_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52767_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52769_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52769_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52772_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52772_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52780_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52780_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52800_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52800_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52804_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52804_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52806_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52806_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52812_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52812_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 52823_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 52823_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 12182_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213
The candidate 12182_fd_Psc-09-Q2b1x1_2026-09-13_03-45-34_20.00sec_0.00C_LIGHT_0213 did not pass the final checks
