This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV
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 08 03.3597 2461255.8597 12.44 01:52:01.37 +11:28:23.6
145.75789 -48.69495 galactic Ari Second-epoch detections are separated by 1.3" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.46 Hestia -1 -0 1 12.5 -0 -0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:52:01.37 +11:28:23.6: 16.19 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:52:01.37 +11:28:23.6: 16.08 +/- 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!
TCP 2026 08 03.3597* 01 52 01.37 +11 28 23.6 12.4 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461255.8597,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260803.3597 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.3597 2461255.8597 12.96 01:41:14.95 +10:37:41.2
142.33382 -50.35774 galactic Psc Second-epoch detections are separated by 1.6" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.124 Alkeste -0 -1 1 13.1 0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:41:14.95 +10:37:41.2: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:41:14.95 +10:37:41.2: 16.00 +/- 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,2461255.8597,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260803.3597 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.3597 2461255.8597 13.53 01:37:09.46 +14:28:17.3
139.25592 -46.94602 galactic Psc Second-epoch detections are separated by 1.8" and 4.3 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 13.8 -0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:37:09.46 +14:28:17.3: 16.19 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:37:09.46 +14:28:17.3: 16.03 +/- 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,2461255.8597,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260803.3597 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.3597 2461255.8597 12.32 01:41:36.47 +15:06:13.3
140.51469 -46.04823 galactic Psc Second-epoch detections are separated by 0.2" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.101 Helena -2 -1 2 12.7 -0 -0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:41:36.47 +15:06:13.3: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:41:36.47 +15:06:13.3: 16.09 +/- 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,2461255.8597,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260803.3597 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
First image: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Last image: 2461255.85997377 03.08.2026 08:38:11.734 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.57
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: 2 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): 6714
Objects passed selection criteria: 6681
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 5028.75
Average stars matched: 4985.25 (99.135 %)
Memory usage VmPeak: 233240 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 29 18:03:05 CDT 2026
VaST build number 1.0rc89-187-gf9db235a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Aug 3 03:41:47 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
First image: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Last image: 2461255.85997377 03.08.2026 08:38:11.734 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 17
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.34
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: 8 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): 36622
Objects passed selection criteria: 36526
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 27312.2
Average stars matched: 26797.8 (98.1162 %)
Memory usage VmPeak: 259988 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 29 18:03:05 CDT 2026
VaST build number 1.0rc89-187-gf9db235a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Aug 3 03:42:29 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
SExtractor catalog cache: saved Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.cat to cache
SExtractor catalog cache: saved Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461255.85946034
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits exists and is non-empty
Saving wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits to local_wcs_cache/
'wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits' -> 'local_wcs_cache/wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits'
wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits exists and is non-empty
Saving wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits to local_wcs_cache/
'wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits' -> 'local_wcs_cache/wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits'
wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits exists and is non-empty
Saving wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits to local_wcs_cache/
'wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits' -> 'local_wcs_cache/wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits'
wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits exists and is non-empty
Saving wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits to local_wcs_cache/
'wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits' -> 'local_wcs_cache/wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (1st reference image)
verification OK: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:46:39.869 +14:00:12.31 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits (1st new image)
verification OK: wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits
Image size: 941.2'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:46:20.711 +13:58:27.51 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:46:39.869 +14:00:12.31
Second-epoch image center 01:46:20.711 +13:58:27.51
Angular distance between the image centers 0.0827 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits (2nd new image)
verification OK: wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
Image size: 941.2'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:46:20.912 +13:58:53.90 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:46:39.869 +14:00:12.31
Second-epoch image center 01:46:20.912 +13:58:53.90
Angular distance between the image centers 0.0797 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 01:46:20.711 +13:58:27.51
Second-epoch second image center 01:46:20.912 +13:58:53.90
Angular distance between the image centers 0.00737 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits &> /tmp/tmp.SkTqeHIUFH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits &> /tmp/tmp.Ckg68WrHNc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits &> /tmp/tmp.xJjrK0XnpZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits &> /tmp/tmp.SivNPcj1cy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
Found non-empty wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
The reference image (wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits) and catalog (wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat) found
'wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat' -> 'wcsmag.cat'
Read 7679 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.3962 to 34.9286 deg, Dec +8.6498 to +19.2740 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 18.3962 to 34.9286 deg, Dec 8.6498 to 19.2740 deg
Loaded 4730 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3851 out of 4065 total matches.
Matched with Tycho-2 4065 out of 7679 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.950100
a=0.000000 b=1.000000 c=22.950100
From vast_summary.log: estimated ref. image limiting mag.: -7.57
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.38
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.38
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7679 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.3962 to 34.9286 deg, Dec +8.6498 to +19.2740 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 18.3962 to 34.9286 deg, Dec 8.6498 to 19.2740 deg
Loaded 4730 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3851 out of 4065 total matches.
Matched with Tycho-2 4065 out of 7679 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Forced-photometry filter: calibrated wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits -> calib.txt_param_ref_wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (aperture=6.0)
Read 6762 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.4566 to 34.9567 deg, Dec +8.6053 to +19.2739 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 18.4566 to 34.9567 deg, Dec 8.6053 to 19.2739 deg
Loaded 4732 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): 3812 out of 4016 total matches.
Matched with Tycho-2 4016 out of 6762 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Forced-photometry filter: calibrated wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits -> calib.txt_param_ref_wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
2.0 pix Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
2.9 pix fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits
2.9 pix fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
Limiting magnitude estimates:
15.4 mag. Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
15.2 mag. Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
13.8 mag. fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits
13.8 mag. fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 11.1 (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
############ /tmp/tmp.SkTqeHIUFH (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_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits' -> 'wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS-calibrated image found: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Checking if the catalog wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS catalog name: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=549, bad_region=0, passed=7679
Got 7679 stars (including 7121 good ones) from the SExtractor catalog wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
util/solve_plate_with_UCAC5 got 7679 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 4876 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 4872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.21"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 7679 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.21"
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 4877 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 7679 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 7679 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
Excluding outliers - 4873 stars left (next iteration limit 5359)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits N_match=4873 sigma_overall_arcsec=0.237 sigma_q1_arcsec=0.323 sigma_q2_arcsec=0.223 sigma_q3_arcsec=0.217 sigma_q4_arcsec=0.200 n_q1=1261 n_q2=1216 n_q3=1199 n_q4=1197 worst_quadrant_to_overall_ratio=1.365
The image catalog is written to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits -region wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Ckg68WrHNc (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_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits' -> 'wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.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-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS-calibrated image found: wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Checking if the catalog wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS catalog name: wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=519, bad_region=0, passed=6762
Got 6762 stars (including 6236 good ones) from the SExtractor catalog wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat
util/solve_plate_with_UCAC5 got 6762 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 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: 4878 matched stars entering correct_measured_positions(), 4878 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 6762 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
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: 4878 matched stars entering correct_measured_positions(), 6762 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 6762 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 4878 stars left (next iteration limit 5365)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits N_match=4878 sigma_overall_arcsec=0.294 sigma_q1_arcsec=0.427 sigma_q2_arcsec=0.270 sigma_q3_arcsec=0.274 sigma_q4_arcsec=0.239 n_q1=1250 n_q2=1227 n_q3=1200 n_q4=1201 worst_quadrant_to_overall_ratio=1.449
The image catalog is written to wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits -region wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.xJjrK0XnpZ (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_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.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_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits
Checking if the catalog wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits
WCS catalog name: wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=231, bad_region=0, passed=2891
Got 2891 stars (including 2658 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits.wcscat
util/solve_plate_with_UCAC5 got 2891 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 490 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 2593 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2591 matched stars entering correct_measured_positions(), 2592 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2591 matched stars entering correct_measured_positions(), 2891 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
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 490 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 2592 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2589 matched stars entering correct_measured_positions(), 2891 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 2589 matched stars entering correct_measured_positions(), 2891 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 2589 stars left (next iteration limit 2850)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2589 robust_rms=10.552 arcsec worst_quadrant_rms=10.891 arcsec
SIP_REFIT: SIP order 3 trial: matched=2589 robust_rms=0.366 arcsec worst_quadrant_rms=0.383 arcsec
SIP_REFIT: SIP order 5 trial: matched=2589 robust_rms=0.288 arcsec worst_quadrant_rms=0.331 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2589 robust_rms_before=0.924 arcsec robust_rms_before_corrected=0.281 arcsec robust_rms_after=0.288 arcsec worst_quadrant_rms_before=0.326 worst_quadrant_rms_after=0.331
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.326 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits N_match=2589 sigma_overall_arcsec=0.271 sigma_q1_arcsec=0.291 sigma_q2_arcsec=0.322 sigma_q3_arcsec=0.240 sigma_q4_arcsec=0.254 n_q1=647 n_q2=633 n_q3=650 n_q4=659 worst_quadrant_to_overall_ratio=1.187
The image catalog is written to wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits -region wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.SivNPcj1cy (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_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.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_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
Checking if the catalog wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
WCS catalog name: wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=221, bad_region=0, passed=2898
Got 2898 stars (including 2674 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits.wcscat
util/solve_plate_with_UCAC5 got 2898 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 2605 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2605 matched stars entering correct_measured_positions(), 2605 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2605 matched stars entering correct_measured_positions(), 2898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
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 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 2605 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2605 matched stars entering correct_measured_positions(), 2898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 2605 matched stars entering correct_measured_positions(), 2898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 2605 stars left (next iteration limit 2865)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2605 robust_rms=10.622 arcsec worst_quadrant_rms=10.877 arcsec
SIP_REFIT: SIP order 3 trial: matched=2605 robust_rms=0.357 arcsec worst_quadrant_rms=0.372 arcsec
SIP_REFIT: SIP order 5 trial: matched=2605 robust_rms=0.276 arcsec worst_quadrant_rms=0.314 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2605 robust_rms_before=0.943 arcsec robust_rms_before_corrected=0.284 arcsec robust_rms_after=0.276 arcsec worst_quadrant_rms_before=0.331 worst_quadrant_rms_after=0.314
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.331 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits N_match=2605 sigma_overall_arcsec=0.290 sigma_q1_arcsec=0.298 sigma_q2_arcsec=0.341 sigma_q3_arcsec=0.271 sigma_q4_arcsec=0.251 n_q1=652 n_q2=639 n_q3=647 n_q4=667 worst_quadrant_to_overall_ratio=1.176
The image catalog is written to wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits -region wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits sigma_overall=0.237 worst_q_ratio=1.365
ref2=Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits sigma_overall=0.294 worst_q_ratio=1.449
new1=fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits sigma_overall=0.271 worst_q_ratio=1.187
new2=fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits sigma_overall=0.290 worst_q_ratio=1.176
reference average sigma_overall=0.2655 worst_q_ratio=1.407
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_astrometric_residuals.png (4873 matched stars from wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.21 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139_astrometric_residuals.png (4878 matched stars from wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.26 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356_astrometric_residuals.png (2589 matched stars from wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357_astrometric_residuals.png (2605 matched stars from wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits'
Saving fully-calibrated image wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits'
Preparing the HTML report for the field Psc-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04646_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357
The candidate 04646_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 01:22:58.49 +12:52:03.9 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 0s
Prepared the HTML report for the field Psc-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
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-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
SExtractor catalog cache: saved Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.cat to cache
SExtractor catalog cache: saved Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Creating symlink local_wcs_cache/wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits exists and is non-empty
wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits exists and is non-empty
wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits exists and is non-empty
wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (1st reference image)
verification OK: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:46:39.869 +14:00:12.31 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits (1st new image)
verification OK: wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits
Image size: 941.2'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:46:20.711 +13:58:27.51 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:46:39.869 +14:00:12.31
Second-epoch image center 01:46:20.711 +13:58:27.51
Angular distance between the image centers 0.0827 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits (2nd new image)
verification OK: wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
Image size: 941.2'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:46:20.912 +13:58:53.90 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:46:39.869 +14:00:12.31
Second-epoch image center 01:46:20.912 +13:58:53.90
Angular distance between the image centers 0.0797 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 01:46:20.711 +13:58:27.51
Second-epoch second image center 01:46:20.912 +13:58:53.90
Angular distance between the image centers 0.00737 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits &> /tmp/tmp.KpP271gMpt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits &> /tmp/tmp.5E8ShreC6u
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits &> /tmp/tmp.Ru5eaX4ByN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits &> /tmp/tmp.12gtuvXeI6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
Found non-empty wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
The reference image (wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits) and catalog (wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat) found
'wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat' -> 'wcsmag.cat'
Read 40639 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.3962 to 34.9791 deg, Dec +8.6321 to +19.2912 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 18.3962 to 34.9791 deg, Dec 8.6321 to 19.2912 deg
Loaded 4752 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): 3678 out of 4107 total matches.
Matched with Tycho-2 4107 out of 40639 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.860050
a=0.000000 b=1.000000 c=22.860050
From vast_summary.log: estimated ref. image limiting mag.: -7.34
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.52
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.52
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 40639 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.3962 to 34.9791 deg, Dec +8.6321 to +19.2912 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 18.3962 to 34.9791 deg, Dec 8.6321 to 19.2912 deg
Loaded 4752 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): 3678 out of 4107 total matches.
Matched with Tycho-2 4107 out of 40639 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Forced-photometry filter: calibrated wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits -> calib.txt_param_ref_wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (aperture=4.9)
Read 38153 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.4016 to 34.9977 deg, Dec +8.5904 to +19.2796 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 18.4016 to 34.9977 deg, Dec 8.5904 to 19.2796 deg
Loaded 4774 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): 3712 out of 4109 total matches.
Matched with Tycho-2 4109 out of 38153 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Forced-photometry filter: calibrated wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits -> calib.txt_param_ref_wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 16 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
1.9 pix Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
2.7 pix fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits
2.7 pix fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
Limiting magnitude estimates:
15.5 mag. Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
15.4 mag. Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
13.9 mag. fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits
13.9 mag. fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 13.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.KpP271gMpt (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_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits' -> 'wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS-calibrated image found: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Checking if the catalog wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS catalog name: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1873, bad_region=4, passed=40626
Got 40626 stars (including 38681 good ones) from the SExtractor catalog wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
util/solve_plate_with_UCAC5 got 40626 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 4881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 4878 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.21"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 40626 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.21"
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 4881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 40626 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.21"
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 40626 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Excluding outliers - 4878 stars left (next iteration limit 5365)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits N_match=4878 sigma_overall_arcsec=0.229 sigma_q1_arcsec=0.300 sigma_q2_arcsec=0.218 sigma_q3_arcsec=0.217 sigma_q4_arcsec=0.197 n_q1=1241 n_q2=1253 n_q3=1190 n_q4=1194 worst_quadrant_to_overall_ratio=1.309
The image catalog is written to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits -region wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.5E8ShreC6u (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_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits' -> 'wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.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-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS-calibrated image found: wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Checking if the catalog wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS catalog name: wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=1585, bad_region=24, passed=38135
Got 38135 stars (including 36454 good ones) from the SExtractor catalog wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat
util/solve_plate_with_UCAC5 got 38135 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4884 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: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4881 matched stars entering correct_measured_positions(), 38135 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
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 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4884 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(), 38135 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 4881 matched stars entering correct_measured_positions(), 38135 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
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-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits N_match=4881 sigma_overall_arcsec=0.286 sigma_q1_arcsec=0.412 sigma_q2_arcsec=0.264 sigma_q3_arcsec=0.267 sigma_q4_arcsec=0.238 n_q1=1246 n_q2=1250 n_q3=1199 n_q4=1186 worst_quadrant_to_overall_ratio=1.439
The image catalog is written to wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits -region wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Ru5eaX4ByN (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_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.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_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits
Checking if the catalog wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits
WCS catalog name: wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=429, bad_region=3, passed=15567
Got 15567 stars (including 15120 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits.wcscat
util/solve_plate_with_UCAC5 got 15567 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 490 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4879 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4876 matched stars entering correct_measured_positions(), 4876 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4876 matched stars entering correct_measured_positions(), 15567 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4878 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4876 matched stars entering correct_measured_positions(), 15567 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4876 matched stars entering correct_measured_positions(), 15567 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4876 stars left (next iteration limit 5363)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits N_match=4876 sigma_overall_arcsec=0.349 sigma_q1_arcsec=0.381 sigma_q2_arcsec=0.400 sigma_q3_arcsec=0.303 sigma_q4_arcsec=0.321 n_q1=1197 n_q2=1135 n_q3=1265 n_q4=1279 worst_quadrant_to_overall_ratio=1.147
The image catalog is written to wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits -region wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.12gtuvXeI6 (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_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.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_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
Checking if the catalog wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
WCS catalog name: wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=443, bad_region=3, passed=15595
Got 15595 stars (including 15130 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits.wcscat
util/solve_plate_with_UCAC5 got 15595 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4883 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 4878 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 15595 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
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: 4879 matched stars entering correct_measured_positions(), 15595 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 15595 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4879 stars left (next iteration limit 5365)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits N_match=4879 sigma_overall_arcsec=0.338 sigma_q1_arcsec=0.376 sigma_q2_arcsec=0.386 sigma_q3_arcsec=0.297 sigma_q4_arcsec=0.304 n_q1=1202 n_q2=1126 n_q3=1281 n_q4=1270 worst_quadrant_to_overall_ratio=1.143
The image catalog is written to wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits -region wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.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_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-37-27_20.00sec_-0.00C_LIGHTs_0356.fits
Saving fully-calibrated image wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.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_2026-08-03_CI_Psc-03-Q1b1x1_033911_TTUQ1b1x1_1686591_Mf9ZVzmV/wcs_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357.fits
Preparing the HTML report for the field Psc-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:41:14.95 +10:37:41.2: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:17:32.58 +14:15:32.1: 11.81 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:31:05.56 +13:26:18.4: 12.92 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:52:01.37 +11:28:23.6: 16.19 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:37:09.46 +14:28:17.3: 16.19 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:41:36.47 +15:06:13.3: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:31:05.56 +13:26:18.4: 12.96 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:41:14.95 +10:37:41.2: 16.00 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:17:32.58 +14:15:32.1: 11.82 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:52:01.37 +11:28:23.6: 16.08 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Forced photometry reference-image weighted average: 11.81 +/- 0.01
Forced photometry filter REJECTED candidate at 01:31:05.56 +13:26:18.4: ref_mag=12.94 +/- 0.02 new_mean_mag=12.9119 delta=0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:17:32.58 +14:15:32.1: ref_mag=11.81 +/- 0.01 new_mean_mag=11.7594 delta=0.05 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:37:09.46 +14:28:17.3: 16.03 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:41:36.47 +15:06:13.3: 16.09 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out17220.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51834.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52000.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 51711_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357
The candidate 51711_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357 did not pass the final checks
Rejecting candidate due to large distance (26.5") between the two second-epoch detections
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Considering the candidate 51745_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357
The candidate 51745_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 51777_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357
The candidate 51777_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357 did not pass the final checks
Rejecting candidate due to large distance (26.5") between the two second-epoch detections
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Considering the candidate 51783_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357
The candidate 51783_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357 did not pass the final checks
Rejecting candidate due to large distance (26.5") between the two second-epoch detections
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Considering the candidate 51796_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357
The candidate 51796_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357 did not pass the final checks
Rejecting candidate due to large distance (26.8") between the two second-epoch detections
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Considering the candidate 51834_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357
Preparing report for the candidate 51834_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357
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Considering the candidate 51890_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357
The candidate 51890_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 01:29:48.26 +18:21:31.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 51900_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357
The candidate 51900_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 51905_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357
The candidate 51905_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 01:39:14.53 +16:36:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51908_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357
Preparing report for the candidate 51908_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357
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Considering the candidate 51910_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357
The candidate 51910_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357 did not pass the final checks
Rejecting candidate due to large distance (26.7") between the two second-epoch detections
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Considering the candidate 51989_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357
The candidate 51989_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357 did not pass the final checks
Rejecting candidate due to large distance (26.7") between the two second-epoch detections
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Considering the candidate 52000_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357
Preparing report for the candidate 52000_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357
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Considering the candidate 36803_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357
The candidate 36803_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 02:10:13.48 +11:32:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17220_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357
Preparing report for the candidate 17220_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357
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Considering the candidate 31656_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357
The candidate 31656_fd_Psc-03-Q1b1x1_2026-08-03_03-38-11_20.00sec_-0.00C_LIGHTs_0357 did not pass the final checks