This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B
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 20.1704 2461180.6704 10.69 11:24:21.47 -11:51:01.8
271.64094 45.66436 galactic Crt Second-epoch detections are separated by 0.1" and 10.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.15 Eunomia -0 -0 0 10.8 0 -0
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:24:21.47 -11:51:01.8: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:24:21.47 -11:51:01.8: 15.55 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461180.6704,10.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260520.1704 10.69CV 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 20.1704 2461180.6704 13.59 11:30:56.29 -08:13:42.9
271.22050 49.62180 galactic Crt Second-epoch detections are separated by 0.8" and 10.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.639 Latona -0 1 1 14.0 0 -0
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:30:56.29 -08:13:42.9: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:30:56.29 -08:13:42.9: 15.66 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461180.6704,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260520.1704 13.59CV 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 20.1704 2461180.6704 13.79 10:54:16.53 -11:15:00.8
262.52527 42.24698 galactic Crt Second-epoch detections are separated by 2.9" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1943 Anteros 19 21 29 13.8 0 -0
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 10:54:16.53 -11:15:00.8: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 10:54:16.53 -11:15:00.8: 15.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461180.6704,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260520.1704 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 20.1704 2461180.6704 12.07 11:12:45.27 -07:17:55.4
264.62272 48.09627 galactic Crt Second-epoch detections are separated by 0.7" and 10.2 pix
The object was found in VSX 1" U Crt
Type: M
# Max. Min./Amp. JD0 Period
9.500 V < 13.500 V 2428269.00000 169.000000000000 M0e
The object was not found in astcheck.
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:12:45.27 -07:17:55.4: 13.09 +/- 0.03 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:12:45.27 -07:17:55.4: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 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
U Crt,2461180.6704,12.07,0.05,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
U Crt 20260520.1704 12.07CV 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: 2461146.71399943 16.04.2026 05:07:59.551 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
First image: 2461146.71399943 16.04.2026 05:07:59.551 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
Last image: 2461180.67071433 20.05.2026 04:05:39.718 /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 9
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.76
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: 3 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): 4870
Objects passed selection criteria: 4862
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 4513.75
Average stars matched: 4394.75 (97.3636 %)
Memory usage VmPeak: 111236 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue May 19 15:05:05 CDT 2026
VaST build number 1.0rc89-63-g0e0f9022
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-19)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue May 19 23:19:53 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: 2461146.71399943 16.04.2026 05:07:59.551 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
First image: 2461146.71399943 16.04.2026 05:07:59.551 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
Last image: 2461180.67071433 20.05.2026 04:05:39.718 /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 40
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.44
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: 10 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): 30200
Objects passed selection criteria: 30130
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 27888.5
Average stars matched: 26919.5 (96.5254 %)
Memory usage VmPeak: 134636 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue May 19 15:05:05 CDT 2026
VaST build number 1.0rc89-63-g0e0f9022
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-19)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue May 19 23:21:14 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/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
SExtractor catalog cache: saved Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat to cache
SExtractor catalog cache: saved Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.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/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.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: 2461180.67010449
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
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits exists and is non-empty
Saving wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits to local_wcs_cache/
'wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits' -> 'local_wcs_cache/wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits'
wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits exists and is non-empty
Saving wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits to local_wcs_cache/
'wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits' -> 'local_wcs_cache/wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits'
wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits exists and is non-empty
Saving wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits to local_wcs_cache/
'wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits' -> 'local_wcs_cache/wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits'
wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits exists and is non-empty
Saving wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits to local_wcs_cache/
'wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits' -> 'local_wcs_cache/wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits (1st reference image)
verification OK: wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.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: 11:08:39.514 -10:01:01.99 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_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits (1st new image)
verification OK: wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 937.0'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:08:36.250 -09:59:07.89 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:39.514 -10:01:01.99
Second-epoch image center 11:08:36.250 -09:59:07.89
Angular distance between the image centers 0.0344 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits (2nd new image)
verification OK: wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 937.0'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:08:38.736 -09:58:19.01 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:39.514 -10:01:01.99
Second-epoch image center 11:08:38.736 -09:58:19.01
Angular distance between the image centers 0.0454 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 11:08:36.250 -09:59:07.89
Second-epoch second image center 11:08:38.736 -09:58:19.01
Angular distance between the image centers 0.01698 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/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits &> /tmp/tmp.zwzJmeZU2M
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits &> /tmp/tmp.KIAbln8Awz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits &> /tmp/tmp.yUCQEijR8R
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits &> /tmp/tmp.rtS9MJD1pY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
Calibrating the magnitude scale
Found non-empty wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.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_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits and wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.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_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits and wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat
Found non-empty wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits and wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat
The reference image (wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits) and catalog (wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat) found
'wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat' -> 'wcsmag.cat'
Read 6296 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 158.7581 to 175.3333 deg, Dec -15.6773 to -4.2200 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 158.7581 to 175.3333 deg, Dec -15.6773 to -4.2200 deg
Loaded 5071 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): 3683 out of 3829 total matches.
Matched with Tycho-2 3829 out of 6296 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.798000
a=0.000000 b=1.000000 c=22.798000
From vast_summary.log: estimated ref. image limiting mag.: -7.76
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.04
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.04
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6296 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 158.7581 to 175.3333 deg, Dec -15.6773 to -4.2200 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 158.7581 to 175.3333 deg, Dec -15.6773 to -4.2200 deg
Loaded 5071 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): 3683 out of 3829 total matches.
Matched with Tycho-2 3829 out of 6296 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits:
Forced-photometry filter: calibrated wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits -> calib.txt_param_ref_wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits (aperture=6.2)
Read 6303 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 158.7581 to 175.3333 deg, Dec -15.6774 to -4.2201 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 158.7581 to 175.3333 deg, Dec -15.6774 to -4.2201 deg
Loaded 5071 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): 3677 out of 3827 total matches.
Matched with Tycho-2 3827 out of 6303 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits:
Forced-photometry filter: calibrated wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits -> calib.txt_param_ref_wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 9 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
2.2 pix Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
2.3 pix fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits
2.3 pix fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
2.1 pix wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
2.2 pix wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
Limiting magnitude estimates:
15.0 mag. Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
15.0 mag. Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
14.8 mag. fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits
14.8 mag. fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 11.8 (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.zwzJmeZU2M (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/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.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_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits' -> 'wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
WCS_IMAGE_NAME=wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
WCS-calibrated image found: wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
Checking if the catalog wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits alredy exist and is non-empty...
Catalog wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
WCS catalog name: wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=454, passed=6296
Got 6296 stars (including 5835 good ones) from the SExtractor catalog wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat
util/solve_plate_with_UCAC5 got 6296 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 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 6214 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 6213 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 6213 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits N_match=964 sigma_overall_arcsec=0.345 sigma_q1_arcsec=0.352 sigma_q2_arcsec=0.408 sigma_q3_arcsec=0.317 sigma_q4_arcsec=0.328 n_q1=225 n_q2=210 n_q3=245 n_q4=284 worst_quadrant_to_overall_ratio=1.184
The image catalog is written to wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits -region wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.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.KIAbln8Awz (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/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.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_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits' -> 'wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
WCS_IMAGE_NAME=wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
WCS-calibrated image found: wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
Checking if the catalog wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits alredy exist and is non-empty...
Catalog wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
WCS catalog name: wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=463, passed=6303
Got 6303 stars (including 5835 good ones) from the SExtractor catalog wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat
util/solve_plate_with_UCAC5 got 6303 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 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 6231 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 6228 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 6228 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits N_match=964 sigma_overall_arcsec=0.340 sigma_q1_arcsec=0.348 sigma_q2_arcsec=0.442 sigma_q3_arcsec=0.302 sigma_q4_arcsec=0.328 n_q1=230 n_q2=201 n_q3=246 n_q4=287 worst_quadrant_to_overall_ratio=1.301
The image catalog is written to wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits -region wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.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.yUCQEijR8R (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_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.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_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits
WCS_IMAGE_NAME=wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits
WCS-calibrated image found: wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits
Checking if the catalog wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits.cat corresponding to the image wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits alredy exist and is non-empty...
Catalog wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits.cat corresponding to the image wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits
WCS catalog name: wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=371, passed=5442
Got 5442 stars (including 5063 good ones) from the SExtractor catalog wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits.cat
util/solve_plate_with_UCAC5 got 5442 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 5392 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 5392 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 5392 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits N_match=962 sigma_overall_arcsec=0.451 sigma_q1_arcsec=0.341 sigma_q2_arcsec=0.638 sigma_q3_arcsec=0.400 sigma_q4_arcsec=0.512 n_q1=233 n_q2=235 n_q3=216 n_q4=278 worst_quadrant_to_overall_ratio=1.415
The image catalog is written to wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits -region wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.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.rtS9MJD1pY (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_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.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_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
WCS_IMAGE_NAME=wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
WCS-calibrated image found: wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
Checking if the catalog wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits.cat corresponding to the image wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits alredy exist and is non-empty...
Catalog wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits.cat corresponding to the image wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
WCS catalog name: wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.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=5422
Got 5422 stars (including 5058 good ones) from the SExtractor catalog wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits.cat
util/solve_plate_with_UCAC5 got 5422 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 5349 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
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 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 5349 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 5349 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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=fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits N_match=959 sigma_overall_arcsec=0.455 sigma_q1_arcsec=0.326 sigma_q2_arcsec=0.630 sigma_q3_arcsec=0.412 sigma_q4_arcsec=0.523 n_q1=228 n_q2=234 n_q3=225 n_q4=272 worst_quadrant_to_overall_ratio=1.384
The image catalog is written to wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits -region wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.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=Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits sigma_overall=0.345 worst_q_ratio=1.184
ref2=Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits sigma_overall=0.340 worst_q_ratio=1.301
new1=fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits sigma_overall=0.451 worst_q_ratio=1.415
new2=fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits sigma_overall=0.455 worst_q_ratio=1.384
reference average sigma_overall=0.3425 worst_q_ratio=1.2425
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142_astrometric_residuals.png (964 matched stars from wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143_astrometric_residuals.png (964 matched stars from wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104_astrometric_residuals.png (962 matched stars from wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105_astrometric_residuals.png (959 matched stars from wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits'
Saving fully-calibrated image wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits'
Preparing the HTML report for the field Crt-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:03:30.71 -06:33:59.4: 12.16 +/- 0.01 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:10:49.33 -09:01:33.5: 12.17 +/- 0.01 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:00:50.72 -09:36:34.8: 12.10 +/- 0.01 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:24:21.47 -11:51:01.8: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:02:57.78 -10:02:14.4: 12.12 +/- 0.01 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:12:45.14 -07:18:00.3: 12.71 +/- 0.02 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:03:39.35 -08:30:12.0: 12.14 +/- 0.01 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:10:49.33 -09:01:33.5: 12.18 +/- 0.01 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:00:50.72 -09:36:34.8: 12.09 +/- 0.01 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:03:30.71 -06:33:59.4: 12.14 +/- 0.01 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:24:21.47 -11:51:01.8: 15.55 +/- 99.00 upperlimit
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:03:39.35 -08:30:12.0: 12.16 +/- 0.01 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:12:45.14 -07:18:00.3: 12.67 +/- 0.02 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:02:57.78 -10:02:14.4: 12.11 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Forced photometry filter REJECTED candidate at 11:10:49.33 -09:01:33.5: ref_mag=12.18 +/- 0.01 new_mean_mag=12.0978 delta=0.08 (need > 0.90)
Forced photometry reference-image weighted average: 12.15 +/- 0.01
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Forced photometry reference-image weighted average: 12.69 +/- 0.02
Forced photometry reference-image weighted average: 12.15 +/- 0.01
Forced photometry filter REJECTED candidate at 11:03:30.71 -06:33:59.4: ref_mag=12.15 +/- 0.01 new_mean_mag=12.0960 delta=0.05 (need > 0.90)
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Forced photometry filter REJECTED candidate at 11:00:50.72 -09:36:34.8: ref_mag=12.09 +/- 0.01 new_mean_mag=12.0443 delta=0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 11:03:39.35 -08:30:12.0: ref_mag=12.15 +/- 0.01 new_mean_mag=12.0795 delta=0.07 (need > 0.90)
Forced photometry filter REJECTED candidate at 11:02:57.78 -10:02:14.4: ref_mag=12.11 +/- 0.01 new_mean_mag=12.0931 delta=0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 11:12:45.14 -07:18:00.3: ref_mag=12.69 +/- 0.02 new_mean_mag=11.9102 delta=0.78 (need > 0.90)
Adding exclusion_list_local.txt__out20318.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20318_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
Preparing report for the candidate 20318_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20385_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 20385_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20386_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 20386_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
**** FOUND 11:06:54.56 -09:29:54.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20403_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 20403_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20405_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 20405_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20406_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 20406_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20407_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 20407_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20408_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 20408_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01696_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 01696_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
**** FOUND 11:01:55.14 -07:39:42.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Crt-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 ####
11:24:21.47 -11:51:01.8
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/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
SExtractor catalog cache: saved Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat to cache
SExtractor catalog cache: saved Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
Creating symlink local_wcs_cache/wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
Creating symlink local_wcs_cache/wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits
Creating symlink local_wcs_cache/wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.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_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits exists and is non-empty
wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits exists and is non-empty
wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits exists and is non-empty
wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits (1st reference image)
verification OK: wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.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: 11:08:39.514 -10:01:01.99 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_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits (1st new image)
verification OK: wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits
Image size: 937.0'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:08:36.250 -09:59:07.89 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:39.514 -10:01:01.99
Second-epoch image center 11:08:36.250 -09:59:07.89
Angular distance between the image centers 0.0344 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits (2nd new image)
verification OK: wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
Image size: 937.0'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:08:38.736 -09:58:19.01 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:39.514 -10:01:01.99
Second-epoch image center 11:08:38.736 -09:58:19.01
Angular distance between the image centers 0.0454 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 11:08:36.250 -09:59:07.89
Second-epoch second image center 11:08:38.736 -09:58:19.01
Angular distance between the image centers 0.01698 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/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits &> /tmp/tmp.QfZJGpxYhM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits &> /tmp/tmp.u6DPH6Qt8O
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits &> /tmp/tmp.o78iiqluAK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits &> /tmp/tmp.1XVsWS07WL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
Calibrating the magnitude scale
Found non-empty wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.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_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits and wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.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_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits and wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat
Found non-empty wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits and wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat
The reference image (wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits) and catalog (wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat) found
'wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat' -> 'wcsmag.cat'
Read 39431 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 158.7287 to 175.3638 deg, Dec -15.6780 to -4.2043 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 158.7287 to 175.3638 deg, Dec -15.6780 to -4.2043 deg
Loaded 5089 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): 3634 out of 3983 total matches.
Matched with Tycho-2 3983 out of 39431 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.670250
a=0.000000 b=1.000000 c=22.670250
From vast_summary.log: estimated ref. image limiting mag.: -7.44
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.23
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.23
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 39431 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 158.7287 to 175.3638 deg, Dec -15.6780 to -4.2043 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 158.7287 to 175.3638 deg, Dec -15.6780 to -4.2043 deg
Loaded 5089 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): 3634 out of 3983 total matches.
Matched with Tycho-2 3983 out of 39431 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits:
Forced-photometry filter: calibrated wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits -> calib.txt_param_ref_wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits (aperture=4.7)
Read 39513 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 158.7263 to 175.3473 deg, Dec -15.6782 to -4.2043 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 158.7263 to 175.3473 deg, Dec -15.6782 to -4.2043 deg
Loaded 5089 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): 3641 out of 3987 total matches.
Matched with Tycho-2 3987 out of 39513 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits:
Forced-photometry filter: calibrated wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits -> calib.txt_param_ref_wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 35 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
2.0 pix Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
2.2 pix fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits
2.2 pix fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
2.0 pix wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
2.0 pix wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
Limiting magnitude estimates:
15.2 mag. Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
15.2 mag. Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
14.8 mag. fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits
14.8 mag. fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 14.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.QfZJGpxYhM (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/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.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_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits' -> 'wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
WCS_IMAGE_NAME=wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
WCS-calibrated image found: wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
Checking if the catalog wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits alredy exist and is non-empty...
Catalog wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
WCS catalog name: wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=1628, passed=39410
Got 39410 stars (including 37728 good ones) from the SExtractor catalog wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat
util/solve_plate_with_UCAC5 got 39410 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 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 38968 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 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 38966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 38967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits N_match=963 sigma_overall_arcsec=0.359 sigma_q1_arcsec=0.324 sigma_q2_arcsec=0.406 sigma_q3_arcsec=0.341 sigma_q4_arcsec=0.331 n_q1=220 n_q2=217 n_q3=246 n_q4=280 worst_quadrant_to_overall_ratio=1.130
The image catalog is written to wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits -region wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.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.u6DPH6Qt8O (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/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.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_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits' -> 'wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
WCS_IMAGE_NAME=wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
WCS-calibrated image found: wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
Checking if the catalog wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits alredy exist and is non-empty...
Catalog wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
WCS catalog name: wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=1588, passed=39493
Got 39493 stars (including 37848 good ones) from the SExtractor catalog wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat
util/solve_plate_with_UCAC5 got 39493 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 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 38958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 38961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 38961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits N_match=964 sigma_overall_arcsec=0.353 sigma_q1_arcsec=0.355 sigma_q2_arcsec=0.447 sigma_q3_arcsec=0.323 sigma_q4_arcsec=0.320 n_q1=222 n_q2=209 n_q3=247 n_q4=286 worst_quadrant_to_overall_ratio=1.267
The image catalog is written to wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits -region wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.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.o78iiqluAK (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_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.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_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits
WCS_IMAGE_NAME=wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits
WCS-calibrated image found: wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits
Checking if the catalog wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits.cat corresponding to the image wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits alredy exist and is non-empty...
Catalog wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits.cat corresponding to the image wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits
WCS catalog name: wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=1624, passed=29662
Got 29662 stars (including 28014 good ones) from the SExtractor catalog wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits.cat
util/solve_plate_with_UCAC5 got 29662 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 29291 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
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 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 29294 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 29294 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits N_match=965 sigma_overall_arcsec=0.450 sigma_q1_arcsec=0.332 sigma_q2_arcsec=0.611 sigma_q3_arcsec=0.381 sigma_q4_arcsec=0.540 n_q1=241 n_q2=228 n_q3=239 n_q4=257 worst_quadrant_to_overall_ratio=1.357
The image catalog is written to wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits -region wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.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.1XVsWS07WL (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_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.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_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
WCS_IMAGE_NAME=wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
WCS-calibrated image found: wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
Checking if the catalog wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits.cat corresponding to the image wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits alredy exist and is non-empty...
Catalog wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits.cat corresponding to the image wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
WCS catalog name: wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1635, passed=29836
Got 29836 stars (including 28168 good ones) from the SExtractor catalog wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits.cat
util/solve_plate_with_UCAC5 got 29836 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.6)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 29341 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.6)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 29342 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 29341 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits N_match=961 sigma_overall_arcsec=0.460 sigma_q1_arcsec=0.327 sigma_q2_arcsec=0.615 sigma_q3_arcsec=0.421 sigma_q4_arcsec=0.514 n_q1=234 n_q2=221 n_q3=248 n_q4=258 worst_quadrant_to_overall_ratio=1.335
The image catalog is written to wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits -region wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.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_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.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_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-04-47_20.00sec_5.00C_LIGHT_0104.fits
Saving fully-calibrated image wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.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_2026-05-19_CI_Crt-01-Q2b1x1_231715_TTUQ2b1x1_459029_d8zd2g0B/wcs_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105.fits
Preparing the HTML report for the field Crt-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 10:54:16.53 -11:15:00.8: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:33:11.32 -12:20:18.4: 13.91 +/- 0.07 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:26:22.09 -06:01:02.1: 14.18 +/- 0.09 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:30:56.29 -08:13:42.9: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:28:37.00 -05:54:33.6: 13.93 +/- 0.07 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:29:26.42 -12:21:37.0: 14.84 +/- 0.17 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:26:32.16 -13:40:34.5: 13.99 +/- 0.08 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 10:54:16.53 -11:15:00.8: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:26:22.09 -06:01:02.1: 14.19 +/- 0.09 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:33:11.32 -12:20:18.4: 13.90 +/- 0.08 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:30:56.29 -08:13:42.9: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:28:37.00 -05:54:33.6: 14.00 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.06
Forced photometry reference-image weighted average: 13.91 +/- 0.05
Forced photometry filter REJECTED candidate at 11:26:22.09 -06:01:02.1: ref_mag=14.18 +/- 0.06 new_mean_mag=14.2223 delta=-0.04 (need > 0.90)
Forced photometry filter REJECTED candidate at 11:33:11.32 -12:20:18.4: ref_mag=13.91 +/- 0.05 new_mean_mag=14.2692 delta=-0.36 (need > 0.90)
Forced photometry reference-image weighted average: 13.96 +/- 0.05
Forced photometry filter REJECTED candidate at 11:28:37.00 -05:54:33.6: ref_mag=13.96 +/- 0.05 new_mean_mag=13.8837 delta=0.08 (need > 0.90)
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:12:32.01 -09:57:18.2: 14.75 +/- 0.13 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:27:15.30 -13:08:32.3: 14.66 +/- 0.14 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:32:19.38 -13:33:34.2: 14.50 +/- 0.14 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:26:32.16 -13:40:34.5: 14.04 +/- 0.08 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:29:26.42 -12:21:37.0: 14.83 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.06
Forced photometry reference-image weighted average: 14.84 +/- 0.12
Forced photometry filter REJECTED candidate at 11:26:32.16 -13:40:34.5: ref_mag=14.01 +/- 0.06 new_mean_mag=13.9223 delta=0.09 (need > 0.90)
Forced photometry filter REJECTED candidate at 11:29:26.42 -12:21:37.0: ref_mag=14.84 +/- 0.12 new_mean_mag=14.4543 delta=0.38 (need > 0.90)
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:12:32.01 -09:57:18.2: 14.82 +/- 0.14 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:27:15.30 -13:08:32.3: 14.75 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.78 +/- 0.10
Forced photometry filter REJECTED candidate at 11:12:32.01 -09:57:18.2: ref_mag=14.78 +/- 0.10 new_mean_mag=14.4706 delta=0.31 (need > 0.90)
Forced photometry reference-image weighted average: 14.70 +/- 0.11
Forced photometry filter REJECTED candidate at 11:27:15.30 -13:08:32.3: ref_mag=14.70 +/- 0.11 new_mean_mag=14.3597 delta=0.34 (need > 0.90)
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:32:19.38 -13:33:34.2: 14.44 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.47 +/- 0.10
Forced photometry filter REJECTED candidate at 11:32:19.38 -13:33:34.2: ref_mag=14.47 +/- 0.10 new_mean_mag=14.4279 delta=0.04 (need > 0.90)
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:29:24.94 -09:13:46.0: 14.73 +/- 0.14 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:30:30.58 -06:59:51.6: 15.00 +/- 0.19 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:27:48.12 -13:48:31.4: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:33:39.89 -12:52:52.0: 14.53 +/- 0.16 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:31:39.58 -10:29:49.0: 14.84 +/- 0.18 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:29:24.94 -09:13:46.0: 14.78 +/- 0.15 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:30:30.58 -06:59:51.6: 15.67 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.75 +/- 0.10
Forced photometry reference-image weighted average: 15.00 +/- 0.19
Forced photometry filter REJECTED candidate at 11:29:24.94 -09:13:46.0: ref_mag=14.75 +/- 0.10 new_mean_mag=14.4580 delta=0.30 (need > 0.90)
Forced photometry filter REJECTED candidate at 11:30:30.58 -06:59:51.6: ref_mag=15.00 +/- 0.19 new_mean_mag=14.5408 delta=0.46 (need > 0.90)
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:25:33.68 -06:24:08.4: 14.68 +/- 0.14 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:24:53.55 -12:24:45.2: 15.14 +/- 0.20 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:14:15.58 -11:18:57.9: 14.89 +/- 0.16 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:27:48.12 -13:48:31.4: 14.84 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.84 +/- 0.18
Forced photometry filter REJECTED candidate at 11:27:48.12 -13:48:31.4: ref_mag=14.84 +/- 0.18 new_mean_mag=14.3623 delta=0.47 (need > 0.90)
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:33:39.89 -12:52:52.0: 14.59 +/- 0.16 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:31:39.58 -10:29:49.0: 14.92 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.56 +/- 0.11
Forced photometry reference-image weighted average: 14.88 +/- 0.13
Forced photometry filter REJECTED candidate at 11:33:39.89 -12:52:52.0: ref_mag=14.56 +/- 0.11 new_mean_mag=14.3492 delta=0.21 (need > 0.90)
Forced photometry filter REJECTED candidate at 11:31:39.58 -10:29:49.0: ref_mag=14.88 +/- 0.13 new_mean_mag=14.5856 delta=0.29 (need > 0.90)
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:25:33.68 -06:24:08.4: 14.77 +/- 0.15 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:24:53.55 -12:24:45.2: 14.85 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.72 +/- 0.10
Forced photometry filter REJECTED candidate at 11:25:33.68 -06:24:08.4: ref_mag=14.72 +/- 0.10 new_mean_mag=14.6671 delta=0.05 (need > 0.90)
Forced photometry reference-image weighted average: 14.96 +/- 0.13
Forced photometry filter REJECTED candidate at 11:24:53.55 -12:24:45.2: ref_mag=14.96 +/- 0.13 new_mean_mag=14.5173 delta=0.44 (need > 0.90)
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:14:15.58 -11:18:57.9: 15.59 +/- 0.30 detection
Forced photometry reference-image weighted average: 15.04 +/- 0.14
Forced photometry filter REJECTED candidate at 11:14:15.58 -11:18:57.9: ref_mag=15.04 +/- 0.14 new_mean_mag=14.6501 delta=0.39 (need > 0.90)
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:28:14.78 -10:45:03.8: 15.03 +/- 0.19 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:09:36.14 -13:29:35.3: 14.82 +/- 0.15 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:18:07.35 -13:23:58.2: 15.09 +/- 0.22 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:17:06.37 -10:32:30.4: 14.71 +/- 0.13 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:24:18.82 -12:22:38.0: 14.51 +/- 0.12 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:28:14.78 -10:45:03.8: 15.15 +/- 0.22 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:09:36.14 -13:29:35.3: 15.13 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.08 +/- 0.14
Forced photometry filter REJECTED candidate at 11:28:14.78 -10:45:03.8: ref_mag=15.08 +/- 0.14 new_mean_mag=14.6734 delta=0.40 (need > 0.90)
Forced photometry reference-image weighted average: 14.94 +/- 0.12
Forced photometry filter REJECTED candidate at 11:09:36.14 -13:29:35.3: ref_mag=14.94 +/- 0.12 new_mean_mag=14.6015 delta=0.34 (need > 0.90)
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:18:07.35 -13:23:58.2: 15.28 +/- 0.26 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:24:18.82 -12:22:38.0: 14.52 +/- 0.12 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:12:45.27 -07:17:55.4: 13.09 +/- 0.03 detection
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:17:06.37 -10:32:30.4: 15.17 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.17 +/- 0.17
Forced photometry filter REJECTED candidate at 11:18:07.35 -13:23:58.2: ref_mag=15.17 +/- 0.17 new_mean_mag=14.7046 delta=0.46 (need > 0.90)
Forced photometry reference-image weighted average: 14.51 +/- 0.08
Forced photometry reference-image weighted average: 14.85 +/- 0.11
Forced photometry filter REJECTED candidate at 11:24:18.82 -12:22:38.0: ref_mag=14.51 +/- 0.08 new_mean_mag=14.6233 delta=-0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 11:17:06.37 -10:32:30.4: ref_mag=14.85 +/- 0.11 new_mean_mag=14.6933 delta=0.16 (need > 0.90)
Forced photometry on wcs_Crt-01-Q2b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:12:45.27 -07:17:55.4: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Forced photometry filter KEPT candidate at 11:12:45.27 -07:17:55.4: ref_mag=13.09 +/- 0.02 new_mean_mag=12.0747 delta=1.01 (need > 0.90)
Adding exclusion_list_local.txt__out08584.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52785.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52926.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 52383_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 52383_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 52384_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 52384_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 52389_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 52389_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
**** FOUND 11:19:02.65 -07:41:29.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52435_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 52435_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
**** FOUND 11:24:21.47 -11:51:01.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52785_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
Preparing report for the candidate 52785_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
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Considering the candidate 52848_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 52848_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
**** FOUND 11:19:30.45 -08:24:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52904_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 52904_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
**** FOUND 10:52:18.62 -11:05:23.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52917_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 52917_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 52926_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
Preparing report for the candidate 52926_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
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Considering the candidate 52927_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 52927_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
**** FOUND 11:01:08.98 -11:39:06.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52970_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 52970_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
**** FOUND 11:23:49.97 -06:16:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53013_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 53013_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
**** FOUND 11:07:30.54 -10:52:09.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53033_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 53033_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 53093_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 53093_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
**** FOUND 11:24:16.67 -11:06:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53104_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 53104_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 53122_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 53122_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 53133_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 53133_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 53148_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 53148_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 53155_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 53155_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 53162_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 53162_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
**** FOUND 11:31:35.42 -08:01:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53168_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 53168_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 53174_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 53174_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 53179_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 53179_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 53185_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 53185_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 53195_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 53195_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 53198_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 53198_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 53212_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 53212_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 53220_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 53220_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 53222_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 53222_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 53227_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 53227_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 53249_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 53249_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 53273_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 53273_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 10397_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 10397_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks
**** FOUND 11:01:55.14 -07:39:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 08584_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
Preparing report for the candidate 08584_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
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Considering the candidate 27574_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105
The candidate 27574_fd_Crt-01-Q2b1x1_2026-05-19_23-05-39_20.00sec_4.90C_LIGHT_0105 did not pass the final checks