This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl
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 11 03.2169 2461347.7169 12.39 01:05:08.55 +13:38:18.8
128.02062 -49.09774 galactic Psc Second-epoch detections are separated by 1.2" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.212 Medea -1 -0 1 12.6 -0 -0
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 01:05:08.55 +13:38:18.8: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 01:05:08.55 +13:38:18.8: 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,2461347.7169,12.39,0.05,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 20261103.2169 12.39CV 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 11 03.2169 2461347.7169 13.37 01:04:44.95 +11:53:42.2
128.09299 -50.84325 galactic Psc Second-epoch detections are separated by 0.3" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.517 Edith -1 -0 1 13.5 -0 0
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 01:04:44.95 +11:53:42.2: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 01:04:44.95 +11:53:42.2: 15.83 +/- 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,2461347.7169,13.37,0.05,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 20261103.2169 13.37CV 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 11 03.2169 2461347.7169 13.79 01:09:11.58 +16:40:48.7
129.05626 -45.98032 galactic Psc Second-epoch detections are separated by 0.4" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1572 Posnania -1 -0 1 13.9 -0 -0
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 01:09:11.58 +16:40:48.7: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 01:09:11.58 +16:40:48.7: 15.78 +/- 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,2461347.7169,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261103.2169 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.2169 2461347.7169 14.28 00:41:04.37 +15:33:13.3
119.25343 -47.24401 galactic Psc Second-epoch detections are separated by 1.5" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.28017 1997 YV13 -2 -2 3 14.7 -0 0
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 00:41:04.37 +15:33:13.3: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 00:41:04.37 +15:33:13.3: 15.40 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.40 +/- 0.24
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,2461347.7169,14.28,0.05,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 20261103.2169 14.28CV 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 11 03.2169 2461347.7169 14.39 00:59:13.59 +17:38:00.4
125.56577 -45.19847 galactic Psc Second-epoch detections are separated by 1.3" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.661 Cloelia -0 -0 0 14.4 0 0
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 00:59:13.59 +17:38:00.4: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 00:59:13.59 +17:38:00.4: 15.82 +/- 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,2461347.7169,14.39,0.05,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 20261103.2169 14.39CV 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: 2461243.89018230 22.07.2026 09:21:41.751 /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
First image: 2461243.89018230 22.07.2026 09:21:41.751 /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
Last image: 2461347.71714222 03.11.2026 05:12:31.088 /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.31
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 35 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): 6990
Objects passed selection criteria: 6951
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 5395.75
Average stars matched: 4681 (86.7535 %)
Memory usage VmPeak: 232736 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.20(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Nov 2 23:56:04 CST 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: 2461243.89018230 22.07.2026 09:21:41.751 /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
First image: 2461243.89018230 22.07.2026 09:21:41.751 /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
Last image: 2461347.71714222 03.11.2026 05:12:31.088 /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 59
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.05
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: 68 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): 36597
Objects passed selection criteria: 36495
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 29552.2
Average stars matched: 25787.5 (87.2607 %)
Memory usage VmPeak: 256032 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.20(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Nov 2 23:59:15 CST 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-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
SExtractor catalog cache: saved Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits.cat to cache
SExtractor catalog cache: saved Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.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-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
Checking WCS cache directory local_wcs_cache
Checking 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: 2461347.71656466
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-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits exists and is non-empty
wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits exists and is non-empty
wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits exists and is non-empty
wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits (1st reference image)
verification OK: wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
Image size: 937.4'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:53:20.923 +13:59:58.60 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-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits (1st new image)
verification OK: wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits
Image size: 937.1'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:53:21.229 +14:00:12.94 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:53:20.923 +13:59:58.60
Second-epoch image center 00:53:21.229 +14:00:12.94
Angular distance between the image centers 0.0042 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits (2nd new image)
verification OK: wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
Image size: 937.1'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: 00:53:21.746 +13:59:42.02 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:53:20.923 +13:59:58.60
Second-epoch image center 00:53:21.746 +13:59:42.02
Angular distance between the image centers 0.0057 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 00:53:21.229 +14:00:12.94
Second-epoch second image center 00:53:21.746 +13:59:42.02
Angular distance between the image centers 0.00884 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-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits &> /tmp/tmp.lo4FAgKPzT
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits &> /tmp/tmp.7PamIwIWZu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits &> /tmp/tmp.CZcIaXIUXO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits &> /tmp/tmp.Y7H3nxkWlc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.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-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits and wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.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-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits and wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits.wcscat
Found non-empty wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits and wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits.wcscat
The reference image (wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits) and catalog (wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits.wcscat) found
'wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits.wcscat' -> 'wcsmag.cat'
Read 6294 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 5.0190 to 21.5394 deg, Dec +8.6191 to +19.2626 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 5.0190 to 21.5394 deg, Dec 8.6191 to 19.2626 deg
Loaded 4654 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): 3742 out of 3856 total matches.
Matched with Tycho-2 3856 out of 6294 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.599200
a=0.000000 b=1.000000 c=22.599200
From vast_summary.log: estimated ref. image limiting mag.: -7.31
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.29
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.29
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6294 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 5.0190 to 21.5394 deg, Dec +8.6191 to +19.2626 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 5.0190 to 21.5394 deg, Dec 8.6191 to 19.2626 deg
Loaded 4654 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): 3742 out of 3856 total matches.
Matched with Tycho-2 3856 out of 6294 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
Forced-photometry filter: calibrated wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits -> calib.txt_param_ref_wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits (aperture=6.2)
Read 6293 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 5.0188 to 21.5394 deg, Dec +8.6193 to +19.2626 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 5.0188 to 21.5394 deg, Dec 8.6193 to 19.2626 deg
Loaded 4654 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): 3741 out of 3855 total matches.
Matched with Tycho-2 3855 out of 6293 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits
Forced-photometry filter: calibrated wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits -> calib.txt_param_ref_wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
2.3 pix Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits
2.2 pix fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits
2.2 pix fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
Limiting magnitude estimates:
15.3 mag. Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
15.3 mag. Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits
15.6 mag. fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits
15.6 mag. fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
All-image limiting magnitude estimate: 15.6 (SNR ) 12.1 (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.lo4FAgKPzT (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_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.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-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits' -> 'wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.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-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
WCS_IMAGE_NAME=wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
WCS-calibrated image found: wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
Checking if the catalog wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits.wcscat corresponding to the image wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits alredy exist and is non-empty...
Catalog wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits.wcscat corresponding to the image wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
WCS catalog name: wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.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=1423, passed=6294
Got 6294 stars (including 4587 good ones) from the SExtractor catalog wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits.wcscat
util/solve_plate_with_UCAC5 got 6294 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4483 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4480 matched stars entering correct_measured_positions(), 4480 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4480 matched stars entering correct_measured_positions(), 5147 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4484 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4481 matched stars entering correct_measured_positions(), 5147 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4481 matched stars entering correct_measured_positions(), 5147 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4481 stars left (next iteration limit 4928)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits N_match=4481 sigma_overall_arcsec=0.353 sigma_q1_arcsec=0.326 sigma_q2_arcsec=0.362 sigma_q3_arcsec=0.369 sigma_q4_arcsec=0.367 n_q1=1314 n_q2=772 n_q3=1516 n_q4=879 worst_quadrant_to_overall_ratio=1.047
WCS_HEADER_DIAG: file=Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits selection=current_pairs N_selected=4481 N_valid=4481 bias_ra_arcsec=0.020 bias_dec_arcsec=0.001 median_sep_arcsec=0.294 p95_sep_arcsec=0.823 n_q1=1314 n_q2=772 n_q3=1516 n_q4=879 occupied_cells_4x4=16/16
The image catalog is written to wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits -region wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.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.7PamIwIWZu (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_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.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-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits' -> 'wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.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-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits
WCS_IMAGE_NAME=wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits
WCS-calibrated image found: wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits
Checking if the catalog wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits.wcscat corresponding to the image wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits alredy exist and is non-empty...
Catalog wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits.wcscat corresponding to the image wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits
WCS catalog name: wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.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=366, bad_region=1434, passed=6293
Got 6293 stars (including 4582 good ones) from the SExtractor catalog wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits.wcscat
util/solve_plate_with_UCAC5 got 6293 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4478 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4473 matched stars entering correct_measured_positions(), 4473 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4473 matched stars entering correct_measured_positions(), 5138 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4479 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4474 matched stars entering correct_measured_positions(), 5138 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4474 matched stars entering correct_measured_positions(), 5138 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4474 stars left (next iteration limit 4920)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits N_match=4474 sigma_overall_arcsec=0.352 sigma_q1_arcsec=0.315 sigma_q2_arcsec=0.352 sigma_q3_arcsec=0.391 sigma_q4_arcsec=0.350 n_q1=1314 n_q2=772 n_q3=1515 n_q4=873 worst_quadrant_to_overall_ratio=1.111
WCS_HEADER_DIAG: file=Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits selection=current_pairs N_selected=4474 N_valid=4474 bias_ra_arcsec=0.020 bias_dec_arcsec=0.011 median_sep_arcsec=0.294 p95_sep_arcsec=0.852 n_q1=1314 n_q2=772 n_q3=1515 n_q4=873 occupied_cells_4x4=16/16
The image catalog is written to wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits -region wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.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.CZcIaXIUXO (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_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.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_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits
WCS_IMAGE_NAME=wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits
WCS-calibrated image found: wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits
Checking if the catalog wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits.wcscat corresponding to the image wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits.wcscat corresponding to the image wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits
WCS catalog name: wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.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=479, bad_region=1784, passed=7780
Got 7780 stars (including 5592 good ones) from the SExtractor catalog wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits.wcscat
util/solve_plate_with_UCAC5 got 7780 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4871 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 4865 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 6352 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 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4872 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 6352 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 6352 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4866 stars left (next iteration limit 5351)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4866 robust_rms=7.623 arcsec worst_region_rms=12.799 arcsec outer_annulus_rms=12.799 arcsec
SIP_REFIT: SIP order 3 trial: matched=4866 robust_rms=0.399 arcsec worst_region_rms=0.877 arcsec outer_annulus_rms=0.877 arcsec
SIP_REFIT: SIP order 5 trial: matched=4866 robust_rms=0.298 arcsec worst_region_rms=0.365 arcsec outer_annulus_rms=0.365 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4866 robust_rms_before=0.913 arcsec robust_rms_before_corrected=0.298 arcsec robust_rms_after=0.298 arcsec worst_region_rms_before=0.355 worst_region_rms_after=0.365 outer_annulus_rms_before=1.385 outer_annulus_rms_after=0.365
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.355 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits worst_region_rms_kept=0.355 arcsec robust_rms_kept=0.298 arcsec matched=4866
WCS_QUALITY_DIAG: file=fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits N_match=4866 sigma_overall_arcsec=0.312 sigma_q1_arcsec=0.294 sigma_q2_arcsec=0.319 sigma_q3_arcsec=0.306 sigma_q4_arcsec=0.325 n_q1=1656 n_q2=956 n_q3=1438 n_q4=816 worst_quadrant_to_overall_ratio=1.043
WCS_HEADER_DIAG: file=fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits selection=current_pairs N_selected=4866 N_valid=4866 bias_ra_arcsec=-0.544 bias_dec_arcsec=0.563 median_sep_arcsec=0.879 p95_sep_arcsec=1.721 n_q1=1656 n_q2=956 n_q3=1438 n_q4=816 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits -region wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.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.Y7H3nxkWlc (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_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.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_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
WCS_IMAGE_NAME=wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
WCS-calibrated image found: wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
Checking if the catalog wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits.wcscat corresponding to the image wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits.wcscat corresponding to the image wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
WCS catalog name: wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.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=481, bad_region=1783, passed=7753
Got 7753 stars (including 5568 good ones) from the SExtractor catalog wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits.wcscat
util/solve_plate_with_UCAC5 got 7753 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4874 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 4868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 6325 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4876 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 6325 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 6325 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4869 stars left (next iteration limit 5354)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4869 robust_rms=7.635 arcsec worst_region_rms=13.019 arcsec outer_annulus_rms=13.019 arcsec
SIP_REFIT: SIP order 3 trial: matched=4869 robust_rms=0.396 arcsec worst_region_rms=0.759 arcsec outer_annulus_rms=0.759 arcsec
SIP_REFIT: SIP order 5 trial: matched=4869 robust_rms=0.305 arcsec worst_region_rms=0.368 arcsec outer_annulus_rms=0.368 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4869 robust_rms_before=0.916 arcsec robust_rms_before_corrected=0.303 arcsec robust_rms_after=0.305 arcsec worst_region_rms_before=0.378 worst_region_rms_after=0.368 outer_annulus_rms_before=1.408 outer_annulus_rms_after=0.368
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.378 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits worst_region_rms_kept=0.378 arcsec robust_rms_kept=0.303 arcsec matched=4869
WCS_QUALITY_DIAG: file=fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits N_match=4869 sigma_overall_arcsec=0.317 sigma_q1_arcsec=0.307 sigma_q2_arcsec=0.303 sigma_q3_arcsec=0.326 sigma_q4_arcsec=0.324 n_q1=1659 n_q2=962 n_q3=1432 n_q4=816 worst_quadrant_to_overall_ratio=1.030
WCS_HEADER_DIAG: file=fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits selection=current_pairs N_selected=4869 N_valid=4869 bias_ra_arcsec=-0.553 bias_dec_arcsec=0.570 median_sep_arcsec=0.886 p95_sep_arcsec=1.710 n_q1=1659 n_q2=962 n_q3=1432 n_q4=816 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits -region wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.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-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits to local_wcs_cache/
'wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits' -> 'local_wcs_cache/wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits'
Saving the final (post-refit) wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits to local_wcs_cache/
'wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits' -> 'local_wcs_cache/wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits'
Saving the final (post-refit) wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits to local_wcs_cache/
'wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits' -> 'local_wcs_cache/wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits'
Saving the final (post-refit) wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits to local_wcs_cache/
'wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits' -> 'local_wcs_cache/wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits sigma_overall=0.353 worst_q_ratio=1.047
ref2=Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits sigma_overall=0.352 worst_q_ratio=1.111
new1=fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits sigma_overall=0.312 worst_q_ratio=1.043
new2=fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits sigma_overall=0.317 worst_q_ratio=1.030
reference average sigma_overall=0.3525 worst_q_ratio=1.079
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418_astrometric_residuals.png (4481 matched stars from wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419_astrometric_residuals.png (4474 matched stars from wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276_astrometric_residuals.png (4866 matched stars from wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277_astrometric_residuals.png (4869 matched stars from wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.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-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits'
Saving fully-calibrated image wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits'
Preparing the HTML report for the field Psc-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Psc-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
SExtractor catalog cache: saved Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits.cat to cache
SExtractor catalog cache: saved Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.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-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
Creating symlink local_wcs_cache/wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
Checking 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-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits exists and is non-empty
wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits exists and is non-empty
wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits exists and is non-empty
wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits (1st reference image)
verification OK: wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
Image size: 937.4'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:53:20.923 +13:59:58.60 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-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits (1st new image)
verification OK: wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits
Image size: 937.1'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:53:21.229 +14:00:12.94 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:53:20.923 +13:59:58.60
Second-epoch image center 00:53:21.229 +14:00:12.94
Angular distance between the image centers 0.0042 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits (2nd new image)
verification OK: wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
Image size: 937.1'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: 00:53:21.746 +13:59:42.02 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:53:20.923 +13:59:58.60
Second-epoch image center 00:53:21.746 +13:59:42.02
Angular distance between the image centers 0.0057 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 00:53:21.229 +14:00:12.94
Second-epoch second image center 00:53:21.746 +13:59:42.02
Angular distance between the image centers 0.00884 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-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits &> /tmp/tmp.AzqC1EdPUt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits &> /tmp/tmp.h3TfzkPN0Z
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits &> /tmp/tmp.iTWyISm4vR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits &> /tmp/tmp.NObMm0TRdu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.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-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits and wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.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-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits and wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits.wcscat
Found non-empty wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits and wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits.wcscat
The reference image (wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits) and catalog (wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits.wcscat) found
'wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits.wcscat' -> 'wcsmag.cat'
Read 33385 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 5.0190 to 21.5394 deg, Dec +8.6084 to +19.2703 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 5.0190 to 21.5394 deg, Dec 8.6084 to 19.2703 deg
Loaded 4659 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): 3709 out of 3992 total matches.
Matched with Tycho-2 3992 out of 33385 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.480700
a=0.000000 b=1.000000 c=22.480700
From vast_summary.log: estimated ref. image limiting mag.: -7.05
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.43
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.43
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 33385 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 5.0190 to 21.5394 deg, Dec +8.6084 to +19.2703 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 5.0190 to 21.5394 deg, Dec 8.6084 to 19.2703 deg
Loaded 4659 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): 3709 out of 3992 total matches.
Matched with Tycho-2 3992 out of 33385 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
Forced-photometry filter: calibrated wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits -> calib.txt_param_ref_wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits (aperture=4.9)
Read 33431 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 5.0188 to 21.5394 deg, Dec +8.6161 to +19.2770 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 5.0188 to 21.5394 deg, Dec 8.6161 to 19.2770 deg
Loaded 4660 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): 3696 out of 3986 total matches.
Matched with Tycho-2 3986 out of 33431 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits
Forced-photometry filter: calibrated wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits -> calib.txt_param_ref_wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 29 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
2.2 pix Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits
2.2 pix fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits
2.2 pix fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
Limiting magnitude estimates:
15.4 mag. Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
15.4 mag. Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits
15.7 mag. fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits
15.7 mag. fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
All-image limiting magnitude estimate: 15.7 (SNR ) 14.6 (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.AzqC1EdPUt (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_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.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-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits' -> 'wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.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-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
WCS_IMAGE_NAME=wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
WCS-calibrated image found: wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
Checking if the catalog wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits.wcscat corresponding to the image wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits alredy exist and is non-empty...
Catalog wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits.wcscat corresponding to the image wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits
WCS catalog name: wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.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=18, blended=1347, bad_region=5852, passed=33367
Got 33367 stars (including 26499 good ones) from the SExtractor catalog wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits.wcscat
util/solve_plate_with_UCAC5 got 33367 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4886 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4881 matched stars entering correct_measured_positions(), 4881 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4881 matched stars entering correct_measured_positions(), 28912 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4886 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4881 matched stars entering correct_measured_positions(), 28912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4881 matched stars entering correct_measured_positions(), 28912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4881 stars left (next iteration limit 5369)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.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-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits N_match=4881 sigma_overall_arcsec=0.355 sigma_q1_arcsec=0.324 sigma_q2_arcsec=0.358 sigma_q3_arcsec=0.376 sigma_q4_arcsec=0.357 n_q1=1487 n_q2=797 n_q3=1612 n_q4=985 worst_quadrant_to_overall_ratio=1.059
WCS_HEADER_DIAG: file=Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits selection=current_pairs N_selected=4881 N_valid=4881 bias_ra_arcsec=0.023 bias_dec_arcsec=-0.008 median_sep_arcsec=0.288 p95_sep_arcsec=0.807 n_q1=1487 n_q2=797 n_q3=1612 n_q4=985 occupied_cells_4x4=16/16
The image catalog is written to wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits -region wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.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.h3TfzkPN0Z (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_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.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-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits' -> 'wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.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-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits
WCS_IMAGE_NAME=wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits
WCS-calibrated image found: wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits
Checking if the catalog wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits.wcscat corresponding to the image wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits alredy exist and is non-empty...
Catalog wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits.wcscat corresponding to the image wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits
WCS catalog name: wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.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=14, blended=1381, bad_region=5894, passed=33417
Got 33417 stars (including 26470 good ones) from the SExtractor catalog wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits.wcscat
util/solve_plate_with_UCAC5 got 33417 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4877 matched stars entering correct_measured_positions(), 4877 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4877 matched stars entering correct_measured_positions(), 28927 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4877 matched stars entering correct_measured_positions(), 28927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4877 matched stars entering correct_measured_positions(), 28927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4877 stars left (next iteration limit 5364)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.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-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits N_match=4877 sigma_overall_arcsec=0.351 sigma_q1_arcsec=0.310 sigma_q2_arcsec=0.351 sigma_q3_arcsec=0.386 sigma_q4_arcsec=0.338 n_q1=1472 n_q2=805 n_q3=1621 n_q4=979 worst_quadrant_to_overall_ratio=1.100
WCS_HEADER_DIAG: file=Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits selection=current_pairs N_selected=4877 N_valid=4877 bias_ra_arcsec=0.025 bias_dec_arcsec=0.002 median_sep_arcsec=0.289 p95_sep_arcsec=0.831 n_q1=1472 n_q2=805 n_q3=1621 n_q4=979 occupied_cells_4x4=16/16
The image catalog is written to wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits -region wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.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.iTWyISm4vR (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_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.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_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits
WCS_IMAGE_NAME=wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits
WCS-calibrated image found: wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits
Checking if the catalog wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits.wcscat corresponding to the image wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits.wcscat corresponding to the image wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits
WCS catalog name: wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.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=16, blended=1735, bad_region=7159, passed=39025
Got 39025 stars (including 30513 good ones) from the SExtractor catalog wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits.wcscat
util/solve_plate_with_UCAC5 got 39025 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4846 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4839 matched stars entering correct_measured_positions(), 4839 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4839 matched stars entering correct_measured_positions(), 33508 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4846 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4838 matched stars entering correct_measured_positions(), 33508 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4838 matched stars entering correct_measured_positions(), 33508 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4838 stars left (next iteration limit 5322)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.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=4838 robust_rms=7.588 arcsec worst_region_rms=12.632 arcsec outer_annulus_rms=12.632 arcsec
SIP_REFIT: SIP order 3 trial: matched=4838 robust_rms=0.401 arcsec worst_region_rms=0.915 arcsec outer_annulus_rms=0.915 arcsec
SIP_REFIT: SIP order 5 trial: matched=4838 robust_rms=0.295 arcsec worst_region_rms=0.361 arcsec outer_annulus_rms=0.361 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4838 robust_rms_before=0.916 arcsec robust_rms_before_corrected=0.293 arcsec robust_rms_after=0.295 arcsec worst_region_rms_before=0.374 worst_region_rms_after=0.361 outer_annulus_rms_before=1.377 outer_annulus_rms_after=0.361
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.374 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits worst_region_rms_kept=0.374 arcsec robust_rms_kept=0.293 arcsec matched=4838
WCS_QUALITY_DIAG: file=fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits N_match=4838 sigma_overall_arcsec=0.307 sigma_q1_arcsec=0.293 sigma_q2_arcsec=0.308 sigma_q3_arcsec=0.310 sigma_q4_arcsec=0.323 n_q1=1654 n_q2=925 n_q3=1430 n_q4=829 worst_quadrant_to_overall_ratio=1.053
WCS_HEADER_DIAG: file=fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits selection=current_pairs N_selected=4838 N_valid=4838 bias_ra_arcsec=-0.544 bias_dec_arcsec=0.569 median_sep_arcsec=0.881 p95_sep_arcsec=1.710 n_q1=1654 n_q2=925 n_q3=1430 n_q4=829 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits -region wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.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.NObMm0TRdu (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_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.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_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
WCS_IMAGE_NAME=wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
WCS-calibrated image found: wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
Checking if the catalog wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits.wcscat corresponding to the image wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits.wcscat corresponding to the image wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
WCS catalog name: wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1732, bad_region=7196, passed=39163
Got 39163 stars (including 30588 good ones) from the SExtractor catalog wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits.wcscat
util/solve_plate_with_UCAC5 got 39163 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4844 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4840 matched stars entering correct_measured_positions(), 4840 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4840 matched stars entering correct_measured_positions(), 33622 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4844 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4839 matched stars entering correct_measured_positions(), 33622 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4839 matched stars entering correct_measured_positions(), 33622 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4839 stars left (next iteration limit 5324)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.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=4839 robust_rms=7.589 arcsec worst_region_rms=13.253 arcsec outer_annulus_rms=13.253 arcsec
SIP_REFIT: SIP order 3 trial: matched=4839 robust_rms=0.395 arcsec worst_region_rms=0.810 arcsec outer_annulus_rms=0.810 arcsec
SIP_REFIT: SIP order 5 trial: matched=4839 robust_rms=0.301 arcsec worst_region_rms=0.368 arcsec outer_annulus_rms=0.368 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4839 robust_rms_before=0.913 arcsec robust_rms_before_corrected=0.303 arcsec robust_rms_after=0.301 arcsec worst_region_rms_before=0.386 worst_region_rms_after=0.368 outer_annulus_rms_before=1.406 outer_annulus_rms_after=0.368
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.386 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits worst_region_rms_kept=0.386 arcsec robust_rms_kept=0.303 arcsec matched=4839
WCS_QUALITY_DIAG: file=fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits N_match=4839 sigma_overall_arcsec=0.318 sigma_q1_arcsec=0.303 sigma_q2_arcsec=0.298 sigma_q3_arcsec=0.324 sigma_q4_arcsec=0.326 n_q1=1670 n_q2=923 n_q3=1417 n_q4=829 worst_quadrant_to_overall_ratio=1.027
WCS_HEADER_DIAG: file=fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits selection=current_pairs N_selected=4839 N_valid=4839 bias_ra_arcsec=-0.550 bias_dec_arcsec=0.576 median_sep_arcsec=0.881 p95_sep_arcsec=1.703 n_q1=1670 n_q2=923 n_q3=1417 n_q4=829 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits -region wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.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-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.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_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-11-41_20.00sec_-0.00C_LIGHT_0276.fits
Saving fully-calibrated image wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.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_2026-11-02_CI_Psc-02-Q2b1x1_233425_TTUQ2b1x1_3494850_L80M1hCl/wcs_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277.fits
Preparing the HTML report for the field Psc-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 01:11:03.91 +10:46:09.3: 14.71 +/- 0.14 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 01:00:37.49 +10:31:24.1: 12.21 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 01:05:59.79 +13:06:38.9: 14.66 +/- 0.12 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 01:05:08.55 +13:38:18.8: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 01:10:23.96 +09:50:39.8: 14.33 +/- 0.10 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 01:09:59.41 +10:21:50.1: 14.23 +/- 0.10 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 01:09:06.85 +09:49:48.4: 14.75 +/- 0.15 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 01:04:44.95 +11:53:42.2: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 00:35:42.84 +10:02:55.5: 13.70 +/- 0.06 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 00:57:45.03 +10:02:41.0: 14.11 +/- 0.08 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 01:00:37.49 +10:31:24.1: 12.23 +/- 0.01 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 01:11:03.91 +10:46:09.3: 14.47 +/- 0.11 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 01:09:59.41 +10:21:50.1: 14.34 +/- 0.10 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 01:05:59.79 +13:06:38.9: 14.62 +/- 0.12 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.01
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 00:35:42.84 +10:02:55.5: 13.65 +/- 0.06 detection
Forced photometry filter REJECTED candidate at 01:00:37.49 +10:31:24.1: ref_mag=12.22 +/- 0.01 new_mean_mag=12.3299 delta=-0.11 (need > 0.90)
Forced photometry reference-image weighted average: 14.57 +/- 0.09
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 00:57:45.03 +10:02:41.0: 14.02 +/- 0.07 detection
Forced photometry filter REJECTED candidate at 01:11:03.91 +10:46:09.3: ref_mag=14.57 +/- 0.09 new_mean_mag=14.5351 delta=0.03 (need > 0.90)
Forced photometry reference-image weighted average: 14.64 +/- 0.09
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 01:05:08.55 +13:38:18.8: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 01:10:23.96 +09:50:39.8: 14.29 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.07
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 01:04:44.95 +11:53:42.2: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 01:09:06.85 +09:49:48.4: 14.74 +/- 0.14 detection
Forced photometry filter REJECTED candidate at 01:05:59.79 +13:06:38.9: ref_mag=14.64 +/- 0.09 new_mean_mag=14.6835 delta=-0.04 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:09:59.41 +10:21:50.1: ref_mag=14.28 +/- 0.07 new_mean_mag=14.5297 delta=-0.25 (need > 0.90)
Forced photometry reference-image weighted average: 13.67 +/- 0.04
Forced photometry reference-image weighted average: 14.06 +/- 0.05
Forced photometry filter REJECTED candidate at 00:57:45.03 +10:02:41.0: ref_mag=14.06 +/- 0.05 new_mean_mag=14.2081 delta=-0.15 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:35:42.84 +10:02:55.5: ref_mag=13.67 +/- 0.04 new_mean_mag=14.1709 delta=-0.50 (need > 0.90)
Forced photometry reference-image weighted average: 14.31 +/- 0.07
Forced photometry reference-image weighted average: 14.74 +/- 0.10
Forced photometry filter REJECTED candidate at 01:10:23.96 +09:50:39.8: ref_mag=14.31 +/- 0.07 new_mean_mag=14.4209 delta=-0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:09:06.85 +09:49:48.4: ref_mag=14.74 +/- 0.10 new_mean_mag=14.6850 delta=0.06 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 00:41:04.37 +15:33:13.3: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 01:11:27.54 +10:16:04.5: 14.53 +/- 0.14 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 01:08:50.10 +14:19:13.9: 14.26 +/- 0.09 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 01:10:34.42 +10:08:22.7: 14.80 +/- 0.15 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 01:09:11.58 +16:40:48.7: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 01:07:14.25 +13:57:18.6: 14.72 +/- 0.13 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 00:59:13.59 +17:38:00.4: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 00:46:20.04 +18:15:13.6: 14.59 +/- 0.13 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 00:41:04.37 +15:33:13.3: 15.40 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.40 +/- 0.24
Forced photometry filter KEPT candidate at 00:41:04.37 +15:33:13.3: ref_mag=15.40 +/- 0.24 new_mean_mag=14.2724 delta=1.13 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 01:08:50.10 +14:19:13.9: 14.23 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.24 +/- 0.06
Forced photometry filter REJECTED candidate at 01:08:50.10 +14:19:13.9: ref_mag=14.24 +/- 0.06 new_mean_mag=14.3666 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 01:07:14.25 +13:57:18.6: 14.68 +/- 0.12 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 01:11:27.54 +10:16:04.5: 14.47 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.70 +/- 0.09
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 01:09:11.58 +16:40:48.7: 15.78 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 01:07:14.25 +13:57:18.6: ref_mag=14.70 +/- 0.09 new_mean_mag=14.5422 delta=0.16 (need > 0.90)
Forced photometry reference-image weighted average: 14.50 +/- 0.10
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 00:46:20.04 +18:15:13.6: 14.69 +/- 0.13 detection
Forced photometry filter REJECTED candidate at 01:11:27.54 +10:16:04.5: ref_mag=14.50 +/- 0.10 new_mean_mag=14.3454 delta=0.16 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 01:10:34.42 +10:08:22.7: 14.87 +/- 0.16 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 00:59:13.59 +17:38:00.4: 15.82 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.64 +/- 0.09
Forced photometry reference-image weighted average: 14.83 +/- 0.11
Forced photometry filter REJECTED candidate at 01:10:34.42 +10:08:22.7: ref_mag=14.83 +/- 0.11 new_mean_mag=14.5138 delta=0.32 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:46:20.04 +18:15:13.6: ref_mag=14.64 +/- 0.09 new_mean_mag=14.5942 delta=0.04 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 00:55:19.70 +12:59:46.6: 14.72 +/- 0.13 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 00:51:18.24 +17:55:38.1: 14.38 +/- 0.10 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 01:09:18.61 +09:59:15.9: 14.73 +/- 0.14 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 01:01:18.76 +11:53:23.9: 14.65 +/- 0.14 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 01:11:13.84 +17:13:57.0: 14.64 +/- 0.12 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 01:11:13.84 +17:13:57.0: 14.86 +/- 0.16 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 00:51:18.24 +17:55:38.1: 14.65 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.72 +/- 0.10
Forced photometry reference-image weighted average: 14.48 +/- 0.08
Forced photometry filter REJECTED candidate at 01:11:13.84 +17:13:57.0: ref_mag=14.72 +/- 0.10 new_mean_mag=14.6998 delta=0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:51:18.24 +17:55:38.1: ref_mag=14.48 +/- 0.08 new_mean_mag=14.4514 delta=0.03 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 01:01:18.76 +11:53:23.9: 14.73 +/- 0.15 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 00:55:19.70 +12:59:46.6: 14.65 +/- 0.12 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 01:09:18.61 +09:59:15.9: 15.41 +/- 0.27 detection
Forced photometry reference-image weighted average: 14.69 +/- 0.10
Forced photometry filter REJECTED candidate at 01:01:18.76 +11:53:23.9: ref_mag=14.69 +/- 0.10 new_mean_mag=14.5976 delta=0.09 (need > 0.90)
Forced photometry reference-image weighted average: 14.68 +/- 0.09
Forced photometry reference-image weighted average: 14.88 +/- 0.13
Forced photometry filter REJECTED candidate at 01:09:18.61 +09:59:15.9: ref_mag=14.88 +/- 0.13 new_mean_mag=14.6400 delta=0.24 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:55:19.70 +12:59:46.6: ref_mag=14.68 +/- 0.09 new_mean_mag=14.5692 delta=0.12 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 00:57:45.41 +15:16:43.8: 14.94 +/- 0.16 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 00:55:38.29 +10:07:17.0: 14.85 +/- 0.16 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 00:36:38.99 +14:54:57.6: 14.91 +/- 0.19 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 00:40:39.51 +16:40:01.7: 14.85 +/- 0.15 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-21-41_20.00sec_5.00C_LIGHT_0418.fits at 00:55:23.78 +10:06:03.9: 15.04 +/- 0.18 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 00:40:39.51 +16:40:01.7: 14.57 +/- 0.12 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 00:36:38.99 +14:54:57.6: 14.57 +/- 0.14 detection
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 00:55:38.29 +10:07:17.0: 15.02 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.69 +/- 0.11
Forced photometry reference-image weighted average: 14.67 +/- 0.09
Forced photometry reference-image weighted average: 14.92 +/- 0.12
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 00:57:45.41 +15:16:43.8: 14.77 +/- 0.14 detection
Forced photometry filter REJECTED candidate at 00:40:39.51 +16:40:01.7: ref_mag=14.67 +/- 0.09 new_mean_mag=14.8010 delta=-0.13 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:36:38.99 +14:54:57.6: ref_mag=14.69 +/- 0.11 new_mean_mag=14.7470 delta=-0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:55:38.29 +10:07:17.0: ref_mag=14.92 +/- 0.12 new_mean_mag=14.6489 delta=0.28 (need > 0.90)
Forced photometry reference-image weighted average: 14.85 +/- 0.10
Forced photometry filter REJECTED candidate at 00:57:45.41 +15:16:43.8: ref_mag=14.85 +/- 0.10 new_mean_mag=14.6551 delta=0.19 (need > 0.90)
Forced photometry on wcs_Psc-02-Q2b1x1_2026-07-22_04-22-19_20.00sec_5.00C_LIGHT_0419.fits at 00:55:23.78 +10:06:03.9: 14.89 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.96 +/- 0.12
Forced photometry filter REJECTED candidate at 00:55:23.78 +10:06:03.9: ref_mag=14.96 +/- 0.12 new_mean_mag=14.8349 delta=0.12 (need > 0.90)
Adding exclusion_list_local.txt__out53203.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54589.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55519.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57755.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 36s
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: 5s
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Considering the candidate 51905_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
The candidate 51905_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277 did not pass the final checks
Rejecting candidate due to large distance (23.8") between the two second-epoch detections
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Considering the candidate 51907_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
The candidate 51907_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277 did not pass the final checks
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Considering the candidate 51908_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
The candidate 51908_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277 did not pass the final checks
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Considering the candidate 51911_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
The candidate 51911_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277 did not pass the final checks
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Considering the candidate 51912_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
The candidate 51912_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277 did not pass the final checks
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Considering the candidate 51913_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
The candidate 51913_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277 did not pass the final checks
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Considering the candidate 51917_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
The candidate 51917_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277 did not pass the final checks
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Considering the candidate 51919_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
The candidate 51919_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277 did not pass the final checks
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Considering the candidate 53145_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
The candidate 53145_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277 did not pass the final checks
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Considering the candidate 53203_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
Preparing report for the candidate 53203_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
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Considering the candidate 54589_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
Preparing report for the candidate 54589_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
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Considering the candidate 55519_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
Preparing report for the candidate 55519_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
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Considering the candidate 56953_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
The candidate 56953_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277 did not pass the final checks
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Considering the candidate 57038_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
Preparing report for the candidate 57038_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
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Considering the candidate 57213_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
The candidate 57213_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277 did not pass the final checks
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Considering the candidate 57282_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
The candidate 57282_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277 did not pass the final checks
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Considering the candidate 57755_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
Preparing report for the candidate 57755_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
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Considering the candidate 57784_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
The candidate 57784_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277 did not pass the final checks
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Considering the candidate 57899_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
The candidate 57899_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277 did not pass the final checks
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Considering the candidate 57906_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
The candidate 57906_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277 did not pass the final checks
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Considering the candidate 58034_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
The candidate 58034_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277 did not pass the final checks
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Considering the candidate 58144_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
The candidate 58144_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277 did not pass the final checks
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Considering the candidate 58249_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
The candidate 58249_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277 did not pass the final checks
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Considering the candidate 58308_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
The candidate 58308_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277 did not pass the final checks
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Considering the candidate 58323_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
The candidate 58323_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277 did not pass the final checks
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Considering the candidate 58376_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
The candidate 58376_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277 did not pass the final checks
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Considering the candidate 58434_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
The candidate 58434_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277 did not pass the final checks
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Considering the candidate 58515_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
The candidate 58515_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277 did not pass the final checks
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Considering the candidate 58516_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277
The candidate 58516_fd_Psc-02-Q2b1x1_2026-11-02_23-12-31_20.00sec_0.00C_LIGHT_0277 did not pass the final checks
