This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 05 14.4451 2461174.9451 10.54 00:59:46.48 +27:56:43.8
125.17662 -34.88991 galactic Psc Second-epoch detections are separated by 0.3" and 3.0 pix
The object was found in VSX 1" W Psc
Type: M
# Max. Min./Amp. JD0 Period
11.400 pg 14.800 pg 2445337.00000 188.100000000000 M2e-M4
The object was not found in astcheck.
Forced photometry on wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:59:46.48 +27:56:43.8: 13.52 +/- 0.03 detection
Forced photometry on wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:59:46.48 +27:56:43.8: 14.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
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
W Psc,2461174.9451,10.54,0.05,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
W Psc 20260514.4451 10.54CV 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 05 14.4451 2461174.9451 10.04 00:47:19.12 +32:41:05.4
121.92928 -30.17890 galactic And Second-epoch detections are separated by 0.9" and 3.0 pix
The object was found in VSX 4" RW And
Type: M
# Max. Min./Amp. JD0 Period
7.900 V 17.300 V 2457251.00000 429.800000000000 M5e-M10e(S6,2e)
The object was not found in astcheck.
Forced photometry on wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:47:19.12 +32:41:05.4: 13.20 +/- 0.03 detection
Forced photometry on wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:47:19.12 +32:41:05.4: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 14.4451* 00 47 19.12 +32 41 05.4 10.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RW And,2461174.9451,10.04,0.05,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
RW And 20260514.4451 10.04CV 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 05 14.4451 2461174.9451 12.13 01:12:13.49 +32:47:10.6
127.97026 -29.88203 galactic Psc Second-epoch detections are separated by 0.4" and 3.0 pix
The object was found in VSX 1" AX Psc
Type: LB:
# Max. Min./Amp. JD0 Period
15.100 pg 16.000 pg 92.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 01:12:13.49 +32:47:10.6: 13.09 +/- 0.02 detection
Forced photometry on wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 01:12:13.49 +32:47:10.6: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
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
AX Psc,2461174.9451,12.13,0.05,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
AX Psc 20260514.4451 12.13CV 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 05 14.4451 2461174.9451 12.66 01:14:27.67 +32:41:38.0
128.52059 -29.92790 galactic Psc Second-epoch detections are separated by 2.9" and 3.2 pix
The object was found in VSX 2" VW Psc
Type: M
# Max. Min./Amp. JD0 Period
14.649 g Y 3.799 g 2444602.00000 296.500000000000 M8/9
The object was not found in astcheck.
Forced photometry on wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 01:14:27.67 +32:41:38.0: 14.29 +/- 0.07 detection
Forced photometry on wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 01:14:27.67 +32:41:38.0: 14.75 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.06
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
VW Psc,2461174.9451,12.66,0.05,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
VW Psc 20260514.4451 12.66CV 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: 2461032.68993344 23.12.2025 04:33:20.249 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
First image: 2461032.68993344 23.12.2025 04:33:20.249 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
Last image: 2461174.94527155 14.05.2026 10:41:01.462 /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.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.: -7.53
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: 71 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): 9454
Objects passed selection criteria: 9416
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 6302.25
Average stars matched: 5928.25 (94.0656 %)
Memory usage VmPeak: 115024 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed May 13 17:47:49 CDT 2026
VaST build number 1.0rc89-54-ga455e386
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-13)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu May 14 06:34:49 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: 2461032.68993344 23.12.2025 04:33:20.249 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
First image: 2461032.68993344 23.12.2025 04:33:20.249 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
Last image: 2461174.94527155 14.05.2026 10:41:01.462 /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.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.: -7.25
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: 64 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): 56539
Objects passed selection criteria: 56374
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 38894
Average stars matched: 36049.2 (92.6859 %)
Memory usage VmPeak: 155760 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed May 13 17:47:49 CDT 2026
VaST build number 1.0rc89-54-ga455e386
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-13)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu May 14 06:40:14 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-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
SExtractor catalog cache: saved Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat to cache
SExtractor catalog cache: saved Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.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-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.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: 2461174.94484606
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-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits exists and is non-empty
Saving wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits to local_wcs_cache/
'wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits' -> 'local_wcs_cache/wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits'
wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits exists and is non-empty
Saving wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits to local_wcs_cache/
'wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits' -> 'local_wcs_cache/wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits'
wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits exists and is non-empty
Saving wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits to local_wcs_cache/
'wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits' -> 'local_wcs_cache/wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits'
wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits exists and is non-empty
Saving wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits to local_wcs_cache/
'wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits' -> 'local_wcs_cache/wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits (1st reference image)
verification OK: wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:59:58.313 +29:59:11.22 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-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits (1st new image)
verification OK: wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits
Image size: 939.1'x624.3' 15.7(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: 01:00:22.925 +30:00:21.56 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:59:58.313 +29:59:11.22
Second-epoch image center 01:00:22.925 +30:00:21.56
Angular distance between the image centers 0.0909 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits (2nd new image)
verification OK: wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
Image size: 939.1'x624.3' 15.7(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: 01:00:24.325 +30:00:22.43 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:59:58.313 +29:59:11.22
Second-epoch image center 01:00:24.325 +30:00:22.43
Angular distance between the image centers 0.0959 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 01:00:22.925 +30:00:21.56
Second-epoch second image center 01:00:24.325 +30:00:22.43
Angular distance between the image centers 0.00506 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-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits &> /tmp/tmp.IFF8hycZmn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits &> /tmp/tmp.qnDN1uhLZv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits &> /tmp/tmp.Lg26Bg99AO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits &> /tmp/tmp.seC4OhHBKP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.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-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits and wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat
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-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits and wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat
Found non-empty wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits and wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat
The reference image (wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits) and catalog (wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat) found
'wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat' -> 'wcsmag.cat'
Read 12201 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 5.5660 to 24.6535 deg, Dec +24.3268 to +35.2840 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 5.5660 to 24.6535 deg, Dec 24.3268 to 35.2840 deg
Loaded 8109 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): 6156 out of 6514 total matches.
Matched with Tycho-2 6514 out of 12201 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.929300
a=0.000000 b=1.000000 c=22.929300
From vast_summary.log: estimated ref. image limiting mag.: -7.53
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 12201 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 5.5660 to 24.6535 deg, Dec +24.3268 to +35.2840 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 5.5660 to 24.6535 deg, Dec 24.3268 to 35.2840 deg
Loaded 8109 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): 6156 out of 6514 total matches.
Matched with Tycho-2 6514 out of 12201 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits:
Forced-photometry filter: calibrated wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits -> calib.txt_param_ref_wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits (aperture=6.0)
Read 11480 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 5.6208 to 24.7112 deg, Dec +24.3682 to +35.3105 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 5.6208 to 24.7112 deg, Dec 24.3682 to 35.3105 deg
Loaded 8115 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): 6080 out of 6460 total matches.
Matched with Tycho-2 6460 out of 11480 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits:
Forced-photometry filter: calibrated wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits -> calib.txt_param_ref_wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits (aperture=5.9)
____ 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-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
2.0 pix Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
2.5 pix fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits
2.4 pix fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
2.1 pix wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
2.0 pix wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
Limiting magnitude estimates:
15.4 mag. Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
15.4 mag. Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
14.0 mag. fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits
14.0 mag. fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.2 (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.IFF8hycZmn (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-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.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_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.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-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.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-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits' -> 'wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
WCS_IMAGE_NAME=wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
WCS-calibrated image found: wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
Checking if the catalog wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat corresponding to the image wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits alredy exist and is non-empty...
Catalog wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat corresponding to the image wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
WCS catalog name: wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=849, passed=12201
Got 12201 stars (including 11339 good ones) from the SExtractor catalog wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat
util/solve_plate_with_UCAC5 got 12201 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 12028 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 12028 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 12028 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits N_match=953 sigma_overall_arcsec=0.314 sigma_q1_arcsec=0.364 sigma_q2_arcsec=0.333 sigma_q3_arcsec=0.300 sigma_q4_arcsec=0.251 n_q1=247 n_q2=259 n_q3=190 n_q4=257 worst_quadrant_to_overall_ratio=1.158
The image catalog is written to wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits -region wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.qnDN1uhLZv (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-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.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_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.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-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.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-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits' -> 'wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
WCS_IMAGE_NAME=wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
WCS-calibrated image found: wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
Checking if the catalog wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.cat corresponding to the image wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits alredy exist and is non-empty...
Catalog wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.cat corresponding to the image wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
WCS catalog name: wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=846, passed=11480
Got 11480 stars (including 10619 good ones) from the SExtractor catalog wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.cat
util/solve_plate_with_UCAC5 got 11480 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
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 11339 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 11337 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 11337 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits N_match=954 sigma_overall_arcsec=0.372 sigma_q1_arcsec=0.470 sigma_q2_arcsec=0.379 sigma_q3_arcsec=0.364 sigma_q4_arcsec=0.305 n_q1=240 n_q2=259 n_q3=196 n_q4=259 worst_quadrant_to_overall_ratio=1.264
The image catalog is written to wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits -region wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Lg26Bg99AO (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_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.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_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits
WCS_IMAGE_NAME=wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits
WCS-calibrated image found: wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits
Checking if the catalog wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits.cat corresponding to the image wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits.cat corresponding to the image wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits
WCS catalog name: wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=356, passed=4457
Got 4457 stars (including 4099 good ones) from the SExtractor catalog wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits.cat
util/solve_plate_with_UCAC5 got 4457 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010434 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 4386 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 4383 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 4383 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 947 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits N_match=947 sigma_overall_arcsec=0.443 sigma_q1_arcsec=0.387 sigma_q2_arcsec=0.567 sigma_q3_arcsec=0.411 sigma_q4_arcsec=0.494 n_q1=257 n_q2=177 n_q3=258 n_q4=255 worst_quadrant_to_overall_ratio=1.278
The image catalog is written to wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits -region wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.seC4OhHBKP (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_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.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_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
WCS_IMAGE_NAME=wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
WCS-calibrated image found: wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
Checking if the catalog wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits.cat corresponding to the image wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits.cat corresponding to the image wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
WCS catalog name: wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits.cat
SExtractor catalog parsing summary: zero_flux=3, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=443, passed=4387
Got 4387 stars (including 3942 good ones) from the SExtractor catalog wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits.cat
util/solve_plate_with_UCAC5 got 4387 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010434 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 4311 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 4311 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 4311 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 949 stars left (next iteration limit 1042)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits N_match=949 sigma_overall_arcsec=0.444 sigma_q1_arcsec=0.393 sigma_q2_arcsec=0.559 sigma_q3_arcsec=0.388 sigma_q4_arcsec=0.529 n_q1=259 n_q2=180 n_q3=253 n_q4=257 worst_quadrant_to_overall_ratio=1.257
The image catalog is written to wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits -region wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits.cat.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-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits sigma_overall=0.314 worst_q_ratio=1.158
ref2=Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits sigma_overall=0.372 worst_q_ratio=1.264
new1=fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits sigma_overall=0.443 worst_q_ratio=1.278
new2=fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits sigma_overall=0.444 worst_q_ratio=1.257
reference average sigma_overall=0.343 worst_q_ratio=1.211
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181_astrometric_residuals.png (953 matched stars from wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096_astrometric_residuals.png (954 matched stars from wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301_astrometric_residuals.png (947 matched stars from wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302_astrometric_residuals.png (949 matched stars from wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits'
Saving fully-calibrated image wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits'
Preparing the HTML report for the field Psc-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:47:19.12 +32:41:05.4: 12.89 +/- 0.02 detection
Forced photometry on wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:59:46.46 +27:56:43.6: 13.38 +/- 0.03 detection
Forced photometry on wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:47:19.12 +32:41:05.4: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Forced photometry filter KEPT candidate at 00:47:19.12 +32:41:05.4: ref_mag=12.73 +/- 0.01 new_mean_mag=9.7014 delta=3.03 (need > 0.90)
Forced photometry on wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:59:46.46 +27:56:43.6: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Forced photometry filter KEPT candidate at 00:59:46.46 +27:56:43.6: ref_mag=13.53 +/- 0.03 new_mean_mag=10.4798 delta=3.05 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out20516.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20758.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
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
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20516_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302
The candidate 20516_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302 did not pass the final checks
**** FOUND 00:47:19.12 +32:41:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.71, MAG_FAINT_SEARCH_LIMIT=10.69)GAIADR2_OUTPUT=# 3.728 361212148368384768 011.82885093981 +32.68560850430 8.2786 7.4230 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.728#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20758_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302
The candidate 20758_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302 did not pass the final checks
**** FOUND 00:59:46.46 +27:56:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.47, MAG_FAINT_SEARCH_LIMIT=11.45)GAIADR2_OUTPUT=# 0.858 307883012627596288 014.94355664546 +27.94568162664 11.1013 9.6718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.858#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 3s
Prepared the HTML report for the field Psc-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
SExtractor catalog cache: saved Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat to cache
SExtractor catalog cache: saved Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.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-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
Creating symlink local_wcs_cache/wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.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-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits exists and is non-empty
wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits exists and is non-empty
wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits exists and is non-empty
wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits (1st reference image)
verification OK: wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:59:58.313 +29:59:11.22 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-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits (1st new image)
verification OK: wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits
Image size: 939.1'x624.3' 15.7(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: 01:00:22.925 +30:00:21.56 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:59:58.313 +29:59:11.22
Second-epoch image center 01:00:22.925 +30:00:21.56
Angular distance between the image centers 0.0909 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits (2nd new image)
verification OK: wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
Image size: 939.1'x624.3' 15.7(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: 01:00:24.325 +30:00:22.43 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:59:58.313 +29:59:11.22
Second-epoch image center 01:00:24.325 +30:00:22.43
Angular distance between the image centers 0.0959 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 01:00:22.925 +30:00:21.56
Second-epoch second image center 01:00:24.325 +30:00:22.43
Angular distance between the image centers 0.00506 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-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits &> /tmp/tmp.Ntclx14MBt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits &> /tmp/tmp.lCQpLg3syZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits &> /tmp/tmp.pSjxjkaEh9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits &> /tmp/tmp.MaZLpcc3XF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.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-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits and wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat
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-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits and wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat
Found non-empty wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits and wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat
The reference image (wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits) and catalog (wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat) found
'wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat' -> 'wcsmag.cat'
Read 67418 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 5.5660 to 24.6789 deg, Dec +24.2962 to +35.2922 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 5.5660 to 24.6789 deg, Dec 24.2962 to 35.2922 deg
Loaded 8148 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): 5658 out of 6593 total matches.
Matched with Tycho-2 6593 out of 67418 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.822200
a=0.000000 b=1.000000 c=22.822200
From vast_summary.log: estimated ref. image limiting mag.: -7.25
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.57
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.57
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 67418 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 5.5660 to 24.6789 deg, Dec +24.2962 to +35.2922 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 5.5660 to 24.6789 deg, Dec 24.2962 to 35.2922 deg
Loaded 8148 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): 5658 out of 6593 total matches.
Matched with Tycho-2 6593 out of 67418 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits:
Forced-photometry filter: calibrated wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits -> calib.txt_param_ref_wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits (aperture=4.8)
Read 69317 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 5.5774 to 24.7112 deg, Dec +24.3307 to +35.3186 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 5.5774 to 24.7112 deg, Dec 24.3307 to 35.3186 deg
Loaded 8155 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): 5653 out of 6601 total matches.
Matched with Tycho-2 6601 out of 69317 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits:
Forced-photometry filter: calibrated wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits -> calib.txt_param_ref_wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 13 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
1.9 pix Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
2.5 pix fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits
2.4 pix fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
2.0 pix wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
1.9 pix wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
Limiting magnitude estimates:
15.6 mag. Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
15.6 mag. Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
14.1 mag. fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits
14.1 mag. fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 13.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Ntclx14MBt (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-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.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_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.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-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.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-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits' -> 'wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
WCS_IMAGE_NAME=wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
WCS-calibrated image found: wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
Checking if the catalog wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat corresponding to the image wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits alredy exist and is non-empty...
Catalog wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat corresponding to the image wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
WCS catalog name: wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=4197, passed=67406
Got 67406 stars (including 63083 good ones) from the SExtractor catalog wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat
util/solve_plate_with_UCAC5 got 67406 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 66697 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
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 66698 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 66698 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits N_match=959 sigma_overall_arcsec=0.300 sigma_q1_arcsec=0.332 sigma_q2_arcsec=0.316 sigma_q3_arcsec=0.252 sigma_q4_arcsec=0.243 n_q1=249 n_q2=256 n_q3=202 n_q4=252 worst_quadrant_to_overall_ratio=1.109
The image catalog is written to wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits -region wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.lCQpLg3syZ (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-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.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_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.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-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.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-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits' -> 'wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
WCS_IMAGE_NAME=wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
WCS-calibrated image found: wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
Checking if the catalog wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.cat corresponding to the image wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits alredy exist and is non-empty...
Catalog wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.cat corresponding to the image wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits
WCS catalog name: wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=4253, passed=69293
Got 69293 stars (including 64940 good ones) from the SExtractor catalog wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.cat
util/solve_plate_with_UCAC5 got 69293 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
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 68378 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 68377 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 68377 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits N_match=959 sigma_overall_arcsec=0.362 sigma_q1_arcsec=0.424 sigma_q2_arcsec=0.384 sigma_q3_arcsec=0.340 sigma_q4_arcsec=0.310 n_q1=244 n_q2=256 n_q3=205 n_q4=254 worst_quadrant_to_overall_ratio=1.171
The image catalog is written to wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits -region wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.pSjxjkaEh9 (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_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.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_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits
WCS_IMAGE_NAME=wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits
WCS-calibrated image found: wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits
Checking if the catalog wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits.cat corresponding to the image wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits.cat corresponding to the image wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits
WCS catalog name: wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=1077, passed=25742
Got 25742 stars (including 24635 good ones) from the SExtractor catalog wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits.cat
util/solve_plate_with_UCAC5 got 25742 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010434 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 25384 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 25385 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 25385 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 950 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits N_match=950 sigma_overall_arcsec=0.457 sigma_q1_arcsec=0.340 sigma_q2_arcsec=0.549 sigma_q3_arcsec=0.417 sigma_q4_arcsec=0.550 n_q1=264 n_q2=176 n_q3=251 n_q4=259 worst_quadrant_to_overall_ratio=1.205
The image catalog is written to wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits -region wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.MaZLpcc3XF (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_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.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_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
WCS_IMAGE_NAME=wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
WCS-calibrated image found: wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
Checking if the catalog wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits.cat corresponding to the image wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits.cat corresponding to the image wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
WCS catalog name: wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits.cat
SExtractor catalog parsing summary: zero_flux=3, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=7, blended=990, passed=26027
Got 26027 stars (including 25009 good ones) from the SExtractor catalog wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits.cat
util/solve_plate_with_UCAC5 got 26027 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010434 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 25677 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 25678 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 25677 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits N_match=949 sigma_overall_arcsec=0.478 sigma_q1_arcsec=0.408 sigma_q2_arcsec=0.563 sigma_q3_arcsec=0.415 sigma_q4_arcsec=0.573 n_q1=266 n_q2=180 n_q3=242 n_q4=261 worst_quadrant_to_overall_ratio=1.199
The image catalog is written to wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits -region wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits.cat.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-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.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_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-40-24_20.00sec_-4.90C_LIGHT_0301.fits
Saving fully-calibrated image wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.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_2026-05-14_CI_Psc-01-Q2b1x1_062603_TTUQ2b1x1_2144441_IcSvmily/wcs_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302.fits
Preparing the HTML report for the field Psc-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:59:25.22 +32:52:26.2: 13.45 +/- 0.04 detection
Forced photometry on wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:45:18.08 +27:56:40.0: 13.05 +/- 0.03 detection
Forced photometry on wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:59:02.64 +32:28:10.4: 13.07 +/- 0.03 detection
Forced photometry on wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:59:46.48 +27:56:43.8: 13.52 +/- 0.03 detection
Forced photometry on wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:59:25.22 +32:52:26.2: 13.41 +/- 0.04 detection
Forced photometry on wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:45:18.08 +27:56:40.0: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Forced photometry filter REJECTED candidate at 00:59:25.22 +32:52:26.2: ref_mag=13.43 +/- 0.03 new_mean_mag=13.1302 delta=0.30 (need > 0.90)
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Forced photometry filter REJECTED candidate at 00:45:18.08 +27:56:40.0: ref_mag=13.06 +/- 0.02 new_mean_mag=12.9341 delta=0.13 (need > 0.90)
Forced photometry on wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:59:02.64 +32:28:10.4: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Forced photometry filter REJECTED candidate at 00:59:02.64 +32:28:10.4: ref_mag=13.08 +/- 0.02 new_mean_mag=12.9716 delta=0.11 (need > 0.90)
Forced photometry on wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 00:47:19.12 +32:41:05.4: 13.20 +/- 0.03 detection
Forced photometry on wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 01:12:13.49 +32:47:10.6: 13.09 +/- 0.02 detection
Forced photometry on wcs_Psc-01-Q2b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits at 01:14:27.67 +32:41:38.0: 14.29 +/- 0.07 detection
Forced photometry on wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:59:46.48 +27:56:43.8: 14.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Forced photometry filter KEPT candidate at 00:59:46.48 +27:56:43.8: ref_mag=13.67 +/- 0.03 new_mean_mag=10.5340 delta=3.14 (need > 0.90)
Forced photometry on wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 00:47:19.12 +32:41:05.4: 12.99 +/- 0.03 detection
Forced photometry on wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 01:12:13.49 +32:47:10.6: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Forced photometry filter KEPT candidate at 00:47:19.12 +32:41:05.4: ref_mag=13.08 +/- 0.02 new_mean_mag=10.0427 delta=3.04 (need > 0.90)
Forced photometry filter KEPT candidate at 01:12:13.49 +32:47:10.6: ref_mag=13.22 +/- 0.02 new_mean_mag=12.1305 delta=1.09 (need > 0.90)
Forced photometry on wcs_Psc-01-Q2b1x1_2026-01-08_21-24-28_20.00sec_-15.00C_LIGHT_0096.fits at 01:14:27.67 +32:41:38.0: 14.75 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.06
Forced photometry filter KEPT candidate at 01:14:27.67 +32:41:38.0: ref_mag=14.41 +/- 0.06 new_mean_mag=12.6630 delta=1.75 (need > 0.90)
Adding exclusion_list_local.txt__out17258.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18503.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out63077.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
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Considering the candidate 83340_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302
The candidate 83340_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 83797_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302
The candidate 83797_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 83953_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302
The candidate 83953_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 85352_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302
The candidate 85352_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302 did not pass the final checks
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Considering the candidate 85542_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302
The candidate 85542_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302 did not pass the final checks
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Considering the candidate 85807_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302
The candidate 85807_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302 did not pass the final checks
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Considering the candidate 86182_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302
The candidate 86182_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302 did not pass the final checks
**** FOUND 01:10:58.92 +31:26:26.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 87989_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302
The candidate 87989_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 88073_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302
The candidate 88073_fd_Psc-01-Q2b1x1_2026-05-14_05-41-01_20.00sec_-4.90C_LIGHT_0302 did not pass the final checks