This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461209.8733,8.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260618.3733 8.13CV 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 06 18.3733 2461209.8733 10.97 23:44:32.46 -04:41:51.1
84.56988 -62.47662 galactic Aqr Second-epoch detections are separated by 0.8" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.192 Nausikaa 0 0 0 11.1 -0 -0
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits at 23:44:32.46 -04:41:51.1: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits at 23:44:32.46 -04:41:51.1: 15.70 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461209.8733,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260618.3733 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461209.8733,8.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260618.3733 8.20CV 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 06 18.3733 2461209.8733 12.90 23:54:25.73 -05:56:48.1
87.75091 -64.84953 galactic Aqr Second-epoch detections are separated by 1.7" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.106 Dione -1 -0 1 13.2 0 0
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits at 23:54:25.73 -05:56:48.1: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits at 23:54:25.73 -05:56:48.1: 15.90 +/- 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,2461209.8733,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260618.3733 12.90CV 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: 2461032.60800240 23.12.2025 02:35:21.407 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
First image: 2461032.60800240 23.12.2025 02:35:21.407 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
Last image: 2461209.87360097 18.06.2026 08:57:49.124 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.74
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: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5149
Objects passed selection criteria: 5131
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: 3779.25
Average stars matched: 3500.25 (92.6176 %)
Memory usage VmPeak: 111060 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jun 16 15:05:04 CDT 2026
VaST build number 1.0rc89-100-g8a7e82c2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jun 18 06:59:55 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: 2461032.60800240 23.12.2025 02:35:21.407 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
First image: 2461032.60800240 23.12.2025 02:35:21.407 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
Last image: 2461209.87360097 18.06.2026 08:57:49.124 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.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.: -7.46
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 15 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 28087
Objects passed selection criteria: 28000
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 21300.5
Average stars matched: 19618.5 (92.1035 %)
Memory usage VmPeak: 129684 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jun 16 15:05:04 CDT 2026
VaST build number 1.0rc89-100-g8a7e82c2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jun 18 07:03:31 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
SExtractor catalog cache: saved Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat to cache
SExtractor catalog cache: saved Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.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-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.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: 2461209.87300578
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-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits exists and is non-empty
Saving wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits to local_wcs_cache/
'wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits' -> 'local_wcs_cache/wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits'
wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits exists and is non-empty
Saving wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits to local_wcs_cache/
'wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits' -> 'local_wcs_cache/wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits'
wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits exists and is non-empty
Saving wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits to local_wcs_cache/
'wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits' -> 'local_wcs_cache/wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits'
wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits exists and is non-empty
Saving wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits to local_wcs_cache/
'wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits' -> 'local_wcs_cache/wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits (1st reference image)
verification OK: wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.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: 23:59:54.531 -02:01:08.13 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-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits (1st new image)
verification OK: wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits
Image size: 938.3'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:00.027 -02:00:19.07 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:54.531 -02:01:08.13
Second-epoch image center 00:00:00.027 -02:00:19.07
Angular distance between the image centers 0.0266 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits (2nd new image)
verification OK: wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
Image size: 938.3'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:02.507 -01:59:34.35 J2000 4789.000 3195.000
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###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:54.531 -02:01:08.13
Second-epoch image center 00:00:02.507 -01:59:34.35
Angular distance between the image centers 0.0422 deg.
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###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 00:00:00.027 -02:00:19.07
Second-epoch second image center 00:00:02.507 -01:59:34.35
Angular distance between the image centers 0.01615 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits &> /tmp/tmp.PVRX1ALcym
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits &> /tmp/tmp.4NPwMgjs8l
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits &> /tmp/tmp.I2eHVWbSfQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits &> /tmp/tmp.KegY1wluZv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.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-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits and wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.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-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits and wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.wcscat
Found non-empty wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits and wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.wcscat
The reference image (wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits) and catalog (wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.wcscat) found
'wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.wcscat' -> 'wcsmag.cat'
Read 6067 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0003 to 359.9989 deg, Dec -7.3208 to +3.2939 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 0.0003 to 359.9989 deg, Dec -7.3208 to 3.2939 deg
Loaded 160398 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): 3377 out of 3518 total matches.
Matched with Tycho-2 3518 out of 6067 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.910100
a=0.000000 b=1.000000 c=22.910100
From vast_summary.log: estimated ref. image limiting mag.: -7.74
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.17
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.17
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6067 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0003 to 359.9989 deg, Dec -7.3208 to +3.2939 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 0.0003 to 359.9989 deg, Dec -7.3208 to 3.2939 deg
Loaded 160398 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): 3377 out of 3518 total matches.
Matched with Tycho-2 3518 out of 6067 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits:
Forced-photometry filter: calibrated wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits -> calib.txt_param_ref_wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits (aperture=6.2)
Read 5991 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0003 to 359.9988 deg, Dec -7.3337 to +3.2897 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 0.0003 to 359.9988 deg, Dec -7.3337 to 3.2897 deg
Loaded 160571 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): 3355 out of 3514 total matches.
Matched with Tycho-2 3514 out of 5991 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits:
Forced-photometry filter: calibrated wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits -> calib.txt_param_ref_wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
2.1 pix Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
2.4 pix fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits
2.4 pix fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
2.1 pix wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
2.1 pix wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
Limiting magnitude estimates:
15.2 mag. Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
15.2 mag. Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
14.4 mag. fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits
14.4 mag. fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.6 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.PVRX1ALcym (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.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-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits' -> 'wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
WCS_IMAGE_NAME=wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
WCS-calibrated image found: wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
Checking if the catalog wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.wcscat corresponding to the image wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits alredy exist and is non-empty...
Catalog wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.wcscat corresponding to the image wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
WCS catalog name: wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=423, passed=6067
Got 6067 stars (including 5634 good ones) from the SExtractor catalog wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.wcscat
util/solve_plate_with_UCAC5 got 6067 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
RA wraps around 0/360 boundary: field RA 352.0769 through 0 to 7.8992, gap 7.8992 to 352.0769
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 5934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.0770 through 0 to 7.8996, gap 7.8996 to 352.0770
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 5932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 5932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits N_match=963 sigma_overall_arcsec=0.309 sigma_q1_arcsec=0.342 sigma_q2_arcsec=0.329 sigma_q3_arcsec=0.334 sigma_q4_arcsec=0.243 n_q1=224 n_q2=259 n_q3=222 n_q4=258 worst_quadrant_to_overall_ratio=1.107
The image catalog is written to wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits -region wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.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.4NPwMgjs8l (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.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-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits' -> 'wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
WCS_IMAGE_NAME=wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
WCS-calibrated image found: wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
Checking if the catalog wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.wcscat corresponding to the image wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits alredy exist and is non-empty...
Catalog wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.wcscat corresponding to the image wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
WCS catalog name: wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=428, passed=5991
Got 5991 stars (including 5551 good ones) from the SExtractor catalog wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.wcscat
util/solve_plate_with_UCAC5 got 5991 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
RA wraps around 0/360 boundary: field RA 352.0704 through 0 to 7.8991, gap 7.8991 to 352.0704
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 5885 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
RA wraps around 0/360 boundary: field RA 352.0705 through 0 to 7.8995, gap 7.8995 to 352.0705
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 5886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 5886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits N_match=962 sigma_overall_arcsec=0.337 sigma_q1_arcsec=0.439 sigma_q2_arcsec=0.340 sigma_q3_arcsec=0.325 sigma_q4_arcsec=0.256 n_q1=220 n_q2=258 n_q3=223 n_q4=261 worst_quadrant_to_overall_ratio=1.305
The image catalog is written to wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits -region wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.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.I2eHVWbSfQ (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_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.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_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits
WCS_IMAGE_NAME=wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits
WCS-calibrated image found: wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits
Checking if the catalog wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits
WCS catalog name: wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=208, passed=3768
Got 3768 stars (including 3558 good ones) from the SExtractor catalog wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits.wcscat
util/solve_plate_with_UCAC5 got 3768 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010426 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1356 through 0 to 7.9485, gap 7.9485 to 352.1356
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 3681 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1357 through 0 to 7.9496, gap 7.9496 to 352.1357
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 3681 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 3681 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits N_match=962 sigma_overall_arcsec=0.410 sigma_q1_arcsec=0.331 sigma_q2_arcsec=0.540 sigma_q3_arcsec=0.339 sigma_q4_arcsec=0.512 n_q1=261 n_q2=208 n_q3=255 n_q4=238 worst_quadrant_to_overall_ratio=1.317
The image catalog is written to wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits -region wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.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.KegY1wluZv (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_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.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_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
WCS_IMAGE_NAME=wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
WCS-calibrated image found: wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
Checking if the catalog wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
WCS catalog name: wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=204, passed=3763
Got 3763 stars (including 3554 good ones) from the SExtractor catalog wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits.wcscat
util/solve_plate_with_UCAC5 got 3763 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010426 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1358 through 0 to 7.9492, gap 7.9492 to 352.1358
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 3673 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1356 through 0 to 7.9499, gap 7.9499 to 352.1356
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 3672 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 3672 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits N_match=962 sigma_overall_arcsec=0.393 sigma_q1_arcsec=0.349 sigma_q2_arcsec=0.550 sigma_q3_arcsec=0.347 sigma_q4_arcsec=0.477 n_q1=261 n_q2=212 n_q3=255 n_q4=234 worst_quadrant_to_overall_ratio=1.401
The image catalog is written to wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits -region wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.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-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits sigma_overall=0.309 worst_q_ratio=1.107
ref2=Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits sigma_overall=0.337 worst_q_ratio=1.305
new1=fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits sigma_overall=0.410 worst_q_ratio=1.317
new2=fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits sigma_overall=0.393 worst_q_ratio=1.401
reference average sigma_overall=0.323 worst_q_ratio=1.206
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057_astrometric_residuals.png (963 matched stars from wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058_astrometric_residuals.png (962 matched stars from wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358_astrometric_residuals.png (962 matched stars from wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359_astrometric_residuals.png (962 matched stars from wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits'
Saving fully-calibrated image wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits'
Preparing the HTML report for the field Psc-08-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits at 23:44:32.46 -04:41:51.1: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits at 23:44:32.46 -04:41:51.1: 15.70 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out20549.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20225_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359
Preparing report for the candidate 20225_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20549_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359
Preparing report for the candidate 20549_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 11s
Prepared the HTML report for the field Psc-08-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
23:44:32.46 -04:41:51.1
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
SExtractor catalog cache: saved Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat to cache
SExtractor catalog cache: saved Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.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-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
Creating symlink local_wcs_cache/wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.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-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits exists and is non-empty
wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits exists and is non-empty
wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits exists and is non-empty
wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits (1st reference image)
verification OK: wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.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: 23:59:54.531 -02:01:08.13 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-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits (1st new image)
verification OK: wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits
Image size: 938.3'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:00.027 -02:00:19.07 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:54.531 -02:01:08.13
Second-epoch image center 00:00:00.027 -02:00:19.07
Angular distance between the image centers 0.0266 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits (2nd new image)
verification OK: wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
Image size: 938.3'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:02.507 -01:59:34.35 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:54.531 -02:01:08.13
Second-epoch image center 00:00:02.507 -01:59:34.35
Angular distance between the image centers 0.0422 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 00:00:00.027 -02:00:19.07
Second-epoch second image center 00:00:02.507 -01:59:34.35
Angular distance between the image centers 0.01615 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits &> /tmp/tmp.pKuuB9Qk7A
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits &> /tmp/tmp.GiWAnYjPPZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits &> /tmp/tmp.qP3spNfu8U
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits &> /tmp/tmp.MharliYc2s
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.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-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits and wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.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-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits and wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.wcscat
Found non-empty wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits and wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.wcscat
The reference image (wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits) and catalog (wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.wcscat) found
'wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.wcscat' -> 'wcsmag.cat'
Read 32031 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0003 to 359.9991 deg, Dec -7.3224 to +3.3002 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 0.0003 to 359.9991 deg, Dec -7.3224 to 3.3002 deg
Loaded 160540 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): 3289 out of 3587 total matches.
Matched with Tycho-2 3587 out of 32031 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.796500
a=0.000000 b=1.000000 c=22.796500
From vast_summary.log: estimated ref. image limiting mag.: -7.46
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.34
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.34
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 32031 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0003 to 359.9991 deg, Dec -7.3224 to +3.3002 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 0.0003 to 359.9991 deg, Dec -7.3224 to 3.3002 deg
Loaded 160540 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): 3289 out of 3587 total matches.
Matched with Tycho-2 3587 out of 32031 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits:
Forced-photometry filter: calibrated wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits -> calib.txt_param_ref_wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits (aperture=4.9)
Read 32121 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0003 to 359.9992 deg, Dec -7.3341 to +3.2914 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 0.0003 to 359.9992 deg, Dec -7.3341 to 3.2914 deg
Loaded 160607 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): 3279 out of 3591 total matches.
Matched with Tycho-2 3591 out of 32121 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits:
Forced-photometry filter: calibrated wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits -> calib.txt_param_ref_wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 14 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
2.0 pix Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
2.3 pix fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits
2.3 pix fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
2.0 pix wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
2.0 pix wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
Limiting magnitude estimates:
15.3 mag. Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
15.3 mag. Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
14.5 mag. fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits
14.5 mag. fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 14.0 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.pKuuB9Qk7A (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.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-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits' -> 'wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
WCS_IMAGE_NAME=wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
WCS-calibrated image found: wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
Checking if the catalog wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.wcscat corresponding to the image wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits alredy exist and is non-empty...
Catalog wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.wcscat corresponding to the image wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
WCS catalog name: wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1283, passed=32021
Got 32021 stars (including 30693 good ones) from the SExtractor catalog wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.wcscat
util/solve_plate_with_UCAC5 got 32021 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
RA wraps around 0/360 boundary: field RA 352.0737 through 0 to 7.9287, gap 7.9287 to 352.0737
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 31504 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.0738 through 0 to 7.9292, gap 7.9292 to 352.0738
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 31503 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 31503 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits N_match=962 sigma_overall_arcsec=0.286 sigma_q1_arcsec=0.328 sigma_q2_arcsec=0.288 sigma_q3_arcsec=0.290 sigma_q4_arcsec=0.231 n_q1=225 n_q2=253 n_q3=226 n_q4=258 worst_quadrant_to_overall_ratio=1.146
The image catalog is written to wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits -region wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.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.GiWAnYjPPZ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.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-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits' -> 'wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
WCS_IMAGE_NAME=wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
WCS-calibrated image found: wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
Checking if the catalog wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.wcscat corresponding to the image wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits alredy exist and is non-empty...
Catalog wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.wcscat corresponding to the image wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
WCS catalog name: wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1325, passed=32107
Got 32107 stars (including 30723 good ones) from the SExtractor catalog wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.wcscat
util/solve_plate_with_UCAC5 got 32107 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
RA wraps around 0/360 boundary: field RA 352.0631 through 0 to 7.9155, gap 7.9155 to 352.0631
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 31619 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
RA wraps around 0/360 boundary: field RA 352.0632 through 0 to 7.9160, gap 7.9160 to 352.0632
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 31619 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 31619 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits N_match=961 sigma_overall_arcsec=0.323 sigma_q1_arcsec=0.428 sigma_q2_arcsec=0.334 sigma_q3_arcsec=0.298 sigma_q4_arcsec=0.249 n_q1=222 n_q2=253 n_q3=230 n_q4=256 worst_quadrant_to_overall_ratio=1.323
The image catalog is written to wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits -region wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.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.qP3spNfu8U (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_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.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_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits
WCS_IMAGE_NAME=wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits
WCS-calibrated image found: wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits
Checking if the catalog wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits
WCS catalog name: wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=845, passed=20175
Got 20175 stars (including 19309 good ones) from the SExtractor catalog wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits.wcscat
util/solve_plate_with_UCAC5 got 20175 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010426 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.0990 through 0 to 7.9485, gap 7.9485 to 352.0990
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 19722 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.0991 through 0 to 7.9495, gap 7.9495 to 352.0991
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 19724 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 19724 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits N_match=960 sigma_overall_arcsec=0.396 sigma_q1_arcsec=0.326 sigma_q2_arcsec=0.518 sigma_q3_arcsec=0.346 sigma_q4_arcsec=0.512 n_q1=264 n_q2=203 n_q3=254 n_q4=239 worst_quadrant_to_overall_ratio=1.309
The image catalog is written to wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits -region wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.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.MharliYc2s (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_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.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_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
WCS_IMAGE_NAME=wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
WCS-calibrated image found: wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
Checking if the catalog wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
WCS catalog name: wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=714, passed=20110
Got 20110 stars (including 19368 good ones) from the SExtractor catalog wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits.wcscat
util/solve_plate_with_UCAC5 got 20110 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010426 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1095 through 0 to 7.9492, gap 7.9492 to 352.1095
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 19705 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1095 through 0 to 7.9499, gap 7.9499 to 352.1095
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 19705 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 19705 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits N_match=960 sigma_overall_arcsec=0.394 sigma_q1_arcsec=0.350 sigma_q2_arcsec=0.546 sigma_q3_arcsec=0.326 sigma_q4_arcsec=0.524 n_q1=264 n_q2=205 n_q3=255 n_q4=236 worst_quadrant_to_overall_ratio=1.385
The image catalog is written to wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits -region wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.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-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.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_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-56-57_20.00sec_4.90C_LIGHT_0358.fits
Saving fully-calibrated image wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.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_2026-06-18_CI_Psc-08-Q2b1x1_043607_TTUQ2b1x1_3273208_bJzpXpVI/wcs_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359.fits
Preparing the HTML report for the field Psc-08-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits at 23:59:45.71 -05:52:34.7: 12.43 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits at 23:54:52.10 +00:04:17.9: 12.72 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits at 23:54:25.73 -05:56:48.1: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits at 00:14:21.58 -02:13:29.7: 12.66 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits at 23:54:53.44 -06:08:35.7: 13.29 +/- 0.03 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits at 00:05:10.84 -05:41:48.0: 12.39 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits at 00:12:34.77 -01:13:42.2: 13.32 +/- 0.04 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits at 00:02:43.71 -03:22:47.0: 13.76 +/- 0.05 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits at 23:57:10.64 -05:26:34.0: 13.61 +/- 0.05 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits at 00:05:10.84 -05:41:48.0: 12.41 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits at 23:59:45.71 -05:52:34.7: 12.42 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits at 23:54:25.73 -05:56:48.1: 15.90 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Forced photometry filter REJECTED candidate at 00:05:10.84 -05:41:48.0: ref_mag=12.40 +/- 0.01 new_mean_mag=12.3474 delta=0.06 (need > 0.90)
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Forced photometry filter REJECTED candidate at 23:59:45.71 -05:52:34.7: ref_mag=12.42 +/- 0.01 new_mean_mag=12.3381 delta=0.09 (need > 0.90)
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits at 23:54:53.44 -06:08:35.7: 13.27 +/- 0.03 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits at 00:14:21.58 -02:13:29.7: 12.63 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits at 23:54:52.10 +00:04:17.9: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter REJECTED candidate at 00:14:21.58 -02:13:29.7: ref_mag=12.65 +/- 0.01 new_mean_mag=12.6177 delta=0.03 (need > 0.90)
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry filter REJECTED candidate at 23:54:53.44 -06:08:35.7: ref_mag=13.28 +/- 0.02 new_mean_mag=13.3641 delta=-0.08 (need > 0.90)
Forced photometry reference-image weighted average: 12.72 +/- 0.02
Forced photometry filter REJECTED candidate at 23:54:52.10 +00:04:17.9: ref_mag=12.72 +/- 0.02 new_mean_mag=12.6289 delta=0.09 (need > 0.90)
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits at 23:57:10.64 -05:26:34.0: 13.59 +/- 0.05 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits at 00:02:43.71 -03:22:47.0: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Forced photometry filter REJECTED candidate at 00:02:43.71 -03:22:47.0: ref_mag=13.65 +/- 0.03 new_mean_mag=13.7517 delta=-0.10 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:57:10.64 -05:26:34.0: ref_mag=13.60 +/- 0.03 new_mean_mag=13.6528 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits at 00:12:34.77 -01:13:42.2: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.03
Forced photometry filter REJECTED candidate at 00:12:34.77 -01:13:42.2: ref_mag=13.37 +/- 0.03 new_mean_mag=13.2739 delta=0.10 (need > 0.90)
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits at 23:46:41.04 -03:59:39.0: 14.10 +/- 0.30 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits at 23:46:41.04 -03:59:39.0: 14.15 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.10 +/- 0.30
Forced photometry filter REJECTED candidate at 23:46:41.04 -03:59:39.0: ref_mag=14.10 +/- 0.30 new_mean_mag=14.2458 delta=-0.15 (need > 0.90)
Adding exclusion_list_local.txt__out53577.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 51721_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359
The candidate 51721_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359 did not pass the final checks
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Considering the candidate 51745_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359
Preparing report for the candidate 51745_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359
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Considering the candidate 52070_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359
The candidate 52070_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359 did not pass the final checks
**** FOUND 23:44:32.47 -04:41:51.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52687_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359
The candidate 52687_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359 did not pass the final checks
**** FOUND 23:42:00.70 +01:48:30.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52969_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359
The candidate 52969_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359 did not pass the final checks
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Considering the candidate 52991_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359
The candidate 52991_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359 did not pass the final checks
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Considering the candidate 53094_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359
The candidate 53094_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359 did not pass the final checks
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Considering the candidate 53230_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359
The candidate 53230_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359 did not pass the final checks
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Considering the candidate 53577_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359
Preparing report for the candidate 53577_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359
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Considering the candidate 53862_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359
The candidate 53862_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359 did not pass the final checks
**** FOUND 00:08:04.87 -02:26:26.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53954_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359
The candidate 53954_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359 did not pass the final checks
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Considering the candidate 54989_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359
The candidate 54989_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359 did not pass the final checks
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Considering the candidate 55090_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359
The candidate 55090_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359 did not pass the final checks
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Considering the candidate 55854_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359
The candidate 55854_fd_Psc-08-Q2b1x1_2026-06-18_03-57-49_20.00sec_5.00C_LIGHT_0359 did not pass the final checks