This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL
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 04 23.2855 2461153.7855 10.27 11:28:17.22 -13:58:29.3
274.21452 44.21129 galactic Crt Second-epoch detections are separated by 0.3" and 1.4 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 -1 1 10.3 0 -0
Forced photometry on wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits at 11:28:17.22 -13:58:29.3: 14.97 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits at 11:28:17.22 -13:58:29.3: 14.95 +/- 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,2461153.7855,10.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260423.2855 10.27CV 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 04 23.2855 2461153.7855 13.12 11:35:08.16 -09:59:08.2
273.85163 48.53047 galactic Crt Second-epoch detections are separated by 1.8" and 1.7 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 0 0 13.6 0 -0
Forced photometry on wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits at 11:35:08.16 -09:59:08.2: 15.32 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits at 11:35:08.16 -09:59:08.2: 15.34 +/- 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,2461153.7855,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260423.2855 13.12CV 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 04 23.2855 2461153.7855 13.30 11:40:44.29 -08:50:03.5
275.00505 50.16451 galactic Crt Second-epoch detections are separated by 1.0" and 1.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.227 Philosophia 0 -0 0 13.2 -0 0
Forced photometry on wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits at 11:40:44.29 -08:50:03.5: 15.30 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits at 11:40:44.29 -08:50:03.5: 15.29 +/- 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,2461153.7855,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260423.2855 13.30CV 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 04 23.2855 2461153.7855 13.66 12:28:44.63 -12:42:49.9
294.34309 49.77905 galactic Crv Second-epoch detections are separated by 1.5" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.36 Atalante 0 -1 1 13.7 -0 0
Forced photometry on wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits at 12:28:44.63 -12:42:49.9: 15.28 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits at 12:28:44.63 -12:42:49.9: 15.25 +/- 0.35 detection
Forced photometry reference-image weighted average: 15.25 +/- 0.35
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,2461153.7855,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260423.2855 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.2855 2461153.7855 13.87 11:44:25.33 -05:16:47.6
273.87745 53.76830 galactic Vir Second-epoch detections are separated by 0.5" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.193 Ambrosia 1 -1 1 14.1 -0 0
Forced photometry on wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits at 11:44:25.33 -05:16:47.6: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits at 11:44:25.33 -05:16:47.6: 15.12 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.12 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 23.2855* 11 44 25.33 -05 16 47.6 13.9 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461153.7855,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260423.2855 13.87CV 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: 2461098.84537233 27.02.2026 08:17:10.169 /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
First image: 2461098.84537233 27.02.2026 08:17:10.169 /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
Last image: 2461153.78584289 23.04.2026 06:51:26.826 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.09
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): 4620
Objects passed selection criteria: 4617
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: 4173.5
Average stars matched: 4034 (96.6575 %)
Memory usage VmPeak: 110512 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 23 01:54:00 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: 2461098.84537233 27.02.2026 08:17:10.169 /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
First image: 2461098.84537233 27.02.2026 08:17:10.169 /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
Last image: 2461153.78584289 23.04.2026 06:51:26.826 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 64
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.81
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 15 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 29338
Objects passed selection criteria: 29272
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: 27235.8
Average stars matched: 26054 (95.661 %)
Memory usage VmPeak: 130732 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 23 01:55:53 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
SExtractor catalog cache: saved Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat to cache
SExtractor catalog cache: saved Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.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/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.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: 2461153.78521382
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits exists and is non-empty
Saving wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits to local_wcs_cache/
'wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits' -> 'local_wcs_cache/wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits'
wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits exists and is non-empty
Saving wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits to local_wcs_cache/
'wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits' -> 'local_wcs_cache/wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits'
wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits exists and is non-empty
Saving wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits to local_wcs_cache/
'wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits' -> 'local_wcs_cache/wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits'
wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits exists and is non-empty
Saving wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits to local_wcs_cache/
'wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits' -> 'local_wcs_cache/wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits (1st reference image)
verification OK: wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
Image size: 941.5'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:59:59.182 -10:00:01.72 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_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits (1st new image)
verification OK: wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 941.3'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: 11:59:57.147 -10:00:20.54 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:59:59.182 -10:00:01.72
Second-epoch image center 11:59:57.147 -10:00:20.54
Angular distance between the image centers 0.0099 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits (2nd new image)
verification OK: wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
Image size: 941.3'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: 11:59:57.503 -10:00:26.92 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:59:59.182 -10:00:01.72
Second-epoch image center 11:59:57.503 -10:00:26.92
Angular distance between the image centers 0.0098 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 11:59:57.147 -10:00:20.54
Second-epoch second image center 11:59:57.503 -10:00:26.92
Angular distance between the image centers 0.00230 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/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits &> /tmp/tmp.ASk8xIKR5K
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits &> /tmp/tmp.dwK5XPgElu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits &> /tmp/tmp.pBPIZRNYWN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits &> /tmp/tmp.IEcAXdrzYk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.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_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits and wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.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_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits and wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat
Found non-empty wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits and wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat
The reference image (wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits) and catalog (wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat) found
'wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat' -> 'wcsmag.cat'
Read 4517 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 171.8751 to 188.0898 deg, Dec -15.2831 to -4.6918 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 171.8751 to 188.0898 deg, Dec -15.2831 to -4.6918 deg
Loaded 4293 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): 3176 out of 3305 total matches.
Matched with Tycho-2 3305 out of 4517 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.861067
a=0.000000 b=1.000000 c=22.861067
From vast_summary.log: estimated ref. image limiting mag.: -8.09
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.77
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.77
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 4517 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 171.8751 to 188.0898 deg, Dec -15.2831 to -4.6918 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 171.8751 to 188.0898 deg, Dec -15.2831 to -4.6918 deg
Loaded 4293 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): 3176 out of 3305 total matches.
Matched with Tycho-2 3305 out of 4517 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits -> calib.txt_param_ref_wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits (aperture=6.0)
Read 4553 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 171.9035 to 188.0897 deg, Dec -15.2830 to -4.6985 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 171.9035 to 188.0897 deg, Dec -15.2830 to -4.6985 deg
Loaded 4276 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): 3188 out of 3300 total matches.
Matched with Tycho-2 3300 out of 4553 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits -> calib.txt_param_ref_wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
2.0 pix Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
2.3 pix fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits
2.2 pix fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
2.0 pix wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
2.0 pix wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
Limiting magnitude estimates:
14.8 mag. Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
14.8 mag. Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
14.7 mag. fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits
14.7 mag. fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 11.5 (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.ASk8xIKR5K (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits' -> 'wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
WCS_IMAGE_NAME=wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
WCS-calibrated image found: wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
Checking if the catalog wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat corresponding to the image wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits alredy exist and is non-empty...
Catalog wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat corresponding to the image wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
WCS catalog name: wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=373, passed=4517
Got 4517 stars (including 4137 good ones) from the SExtractor catalog wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat
util/solve_plate_with_UCAC5 got 4517 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 4478 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 4477 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 4477 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits -region wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.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.dwK5XPgElu (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits' -> 'wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
WCS_IMAGE_NAME=wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
WCS-calibrated image found: wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
Checking if the catalog wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat corresponding to the image wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits alredy exist and is non-empty...
Catalog wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat corresponding to the image wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
WCS catalog name: wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=364, passed=4553
Got 4553 stars (including 4187 good ones) from the SExtractor catalog wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat
util/solve_plate_with_UCAC5 got 4553 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 4508 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 4509 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 4509 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits -region wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.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.pBPIZRNYWN (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_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.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_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits
WCS_IMAGE_NAME=wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits
WCS-calibrated image found: wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits
Checking if the catalog wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits.cat corresponding to the image wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits.cat corresponding to the image wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits
WCS catalog name: wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=263, passed=3953
Got 3953 stars (including 3685 good ones) from the SExtractor catalog wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits.cat
util/solve_plate_with_UCAC5 got 3953 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 3913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 3915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 3915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits -region wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.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.IEcAXdrzYk (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_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.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_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
WCS_IMAGE_NAME=wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
WCS-calibrated image found: wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
Checking if the catalog wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits.cat corresponding to the image wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits.cat corresponding to the image wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
WCS catalog name: wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=253, passed=3786
Got 3786 stars (including 3529 good ones) from the SExtractor catalog wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits.cat
util/solve_plate_with_UCAC5 got 3786 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 968 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 3746 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 3745 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 3745 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits -region wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits'
Saving fully-calibrated image wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits'
Preparing the HTML report for the field Vir-10-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20283.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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 20283_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
Preparing report for the candidate 20283_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 8s
Prepared the HTML report for the field Vir-10-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
11:28:17.22 -13:58:29.3
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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
SExtractor catalog cache: saved Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat to cache
SExtractor catalog cache: saved Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
Creating symlink local_wcs_cache/wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.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_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits exists and is non-empty
wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits exists and is non-empty
wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits exists and is non-empty
wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits (1st reference image)
verification OK: wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
Image size: 941.5'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:59:59.182 -10:00:01.72 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_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits (1st new image)
verification OK: wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits
Image size: 941.3'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: 11:59:57.147 -10:00:20.54 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:59:59.182 -10:00:01.72
Second-epoch image center 11:59:57.147 -10:00:20.54
Angular distance between the image centers 0.0099 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits (2nd new image)
verification OK: wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
Image size: 941.3'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: 11:59:57.503 -10:00:26.92 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:59:59.182 -10:00:01.72
Second-epoch image center 11:59:57.503 -10:00:26.92
Angular distance between the image centers 0.0098 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 11:59:57.147 -10:00:20.54
Second-epoch second image center 11:59:57.503 -10:00:26.92
Angular distance between the image centers 0.00230 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/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits &> /tmp/tmp.ZaRerjMu6y
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits &> /tmp/tmp.Dpypj2D1Db
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits &> /tmp/tmp.hEHTvAPMVw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits &> /tmp/tmp.E6c5Dq3zfs
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.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_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits and wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.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_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits and wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat
Found non-empty wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits and wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat
The reference image (wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits) and catalog (wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat) found
'wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat' -> 'wcsmag.cat'
Read 29056 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 171.8751 to 188.1080 deg, Dec -15.2896 to -4.6877 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 171.8751 to 188.1080 deg, Dec -15.2896 to -4.6877 deg
Loaded 4301 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): 3518 out of 3765 total matches.
Matched with Tycho-2 3765 out of 29056 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.705276
a=0.000000 b=1.000000 c=22.705276
From vast_summary.log: estimated ref. image limiting mag.: -7.81
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.90
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.90
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 29056 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 171.8751 to 188.1080 deg, Dec -15.2896 to -4.6877 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 171.8751 to 188.1080 deg, Dec -15.2896 to -4.6877 deg
Loaded 4301 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): 3518 out of 3765 total matches.
Matched with Tycho-2 3765 out of 29056 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits -> calib.txt_param_ref_wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits (aperture=4.6)
Read 28855 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 171.8772 to 188.1252 deg, Dec -15.2945 to -4.6933 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 171.8772 to 188.1252 deg, Dec -15.2945 to -4.6933 deg
Loaded 4301 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): 3530 out of 3758 total matches.
Matched with Tycho-2 3758 out of 28855 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits -> calib.txt_param_ref_wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 55 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.9 pix Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
1.9 pix Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
2.1 pix fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits
2.0 pix fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
1.9 pix wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
1.9 pix wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
Limiting magnitude estimates:
14.9 mag. Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
14.9 mag. Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
14.8 mag. fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits
14.7 mag. fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.0 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ZaRerjMu6y (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits' -> 'wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
WCS_IMAGE_NAME=wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
WCS-calibrated image found: wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
Checking if the catalog wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat corresponding to the image wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits alredy exist and is non-empty...
Catalog wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat corresponding to the image wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
WCS catalog name: wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1008, passed=29048
Got 29048 stars (including 27997 good ones) from the SExtractor catalog wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat
util/solve_plate_with_UCAC5 got 29048 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 28818 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 28817 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 28817 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits -region wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-10-Q1b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.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.Dpypj2D1Db (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits' -> 'wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
WCS_IMAGE_NAME=wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
WCS-calibrated image found: wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
Checking if the catalog wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat corresponding to the image wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits alredy exist and is non-empty...
Catalog wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat corresponding to the image wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
WCS catalog name: wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1003, passed=28852
Got 28852 stars (including 27808 good ones) from the SExtractor catalog wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat
util/solve_plate_with_UCAC5 got 28852 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 28570 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 28569 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 28569 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits -region wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-10-Q1b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.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.hEHTvAPMVw (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_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.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_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits
WCS_IMAGE_NAME=wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits
WCS-calibrated image found: wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits
Checking if the catalog wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits.cat corresponding to the image wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits.cat corresponding to the image wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits
WCS catalog name: wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=773, passed=25863
Got 25863 stars (including 25051 good ones) from the SExtractor catalog wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits.cat
util/solve_plate_with_UCAC5 got 25863 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 431 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 25696 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 25696 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 25696 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits -region wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.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.E6c5Dq3zfs (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_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.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_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
WCS_IMAGE_NAME=wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
WCS-calibrated image found: wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
Checking if the catalog wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits.cat corresponding to the image wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits.cat corresponding to the image wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
WCS catalog name: wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=731, passed=25964
Got 25964 stars (including 25194 good ones) from the SExtractor catalog wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits.cat
util/solve_plate_with_UCAC5 got 25964 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 431 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 25747 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 25752 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 25752 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits -region wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.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_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-50-32_20.00sec_-4.90C_LIGHTs_0128.fits
Saving fully-calibrated image wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.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_2026-04-23_CI_Vir-10-Q1b1x1_015223_TTUQ1b1x1_577926_FJSveMtL/wcs_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129.fits
Preparing the HTML report for the field Vir-10-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out32117.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32118.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32805.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32852.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32856.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32870.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out33057.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out33070.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out33115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out33210.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out33243.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out32487.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32602.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32833.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 32110_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32110_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 11:32:52.29 -11:50:37.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32113_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32113_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 12:21:34.59 -10:02:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32115_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32115_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 11:55:29.13 -06:25:22.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32116_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32116_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 11:41:16.49 -06:30:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32117_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32117_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 12:26:10.17 -09:37:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 1.242 3579571880749764864 186.54272365894 -09.63041872631 13.2540 12.7016 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.242#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32118_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32118_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 11:41:35.95 -09:49:57.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)
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Considering the candidate 32154_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32154_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 11:28:17.24 -13:58:29.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 32158_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32158_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 32224_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32224_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 32247_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32247_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 32260_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32260_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 32305_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32305_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 32359_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32359_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 32385_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32385_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 32417_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32417_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 32418_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32418_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 32427_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32427_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 32447_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32447_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 32475_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32475_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 32487_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
Preparing report for the candidate 32487_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
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Considering the candidate 32558_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32558_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 32563_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
Preparing report for the candidate 32563_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
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Considering the candidate 32602_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
Preparing report for the candidate 32602_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
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Considering the candidate 32738_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32738_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 11:34:47.09 -11:45:29.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32770_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32770_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 32781_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32781_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 11:28:51.33 -11:18:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32788_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32788_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 12:22:01.34 -09:21:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32796_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32796_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 12:29:27.01 -12:26:26.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32805_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32805_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 11:37:20.69 -14:38:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 1.494 3548832765453528192 174.33636508396 -14.64352506228 14.4370 13.9533 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.494#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32833_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
Preparing report for the candidate 32833_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
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Considering the candidate 32837_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32837_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 12:23:29.93 -11:48:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32843_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32843_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 12:25:29.92 -06:47:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32852_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32852_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 12:28:27.27 -05:46:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 1.326 3680571129091810816 187.11398592779 -05.76958147270 14.4046 13.7659 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.326#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32856_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32856_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 12:30:25.09 -06:11:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 1.810 3679747526163035520 187.60458522514 -06.18961196183 14.5167 13.8654 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.810#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32857_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32857_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 11:39:48.32 -14:30:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32861_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32861_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 11:29:59.54 -12:44:13.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32869_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32869_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 12:16:03.92 -13:25:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32870_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32870_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 12:27:22.54 -09:01:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 1.868 3579739143956068352 186.84345533914 -09.02083147199 14.5425 13.9629 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.868#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32885_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32885_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 12:24:59.91 -07:12:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32888_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32888_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 12:26:26.59 -12:30:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32901_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32901_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 12:27:29.44 -06:10:56.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32906_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32906_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 12:27:14.73 -10:05:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32933_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32933_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 12:25:55.72 -06:06:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32997_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 32997_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 11:39:43.20 -11:44:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33020_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 33020_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 11:31:47.91 -08:59:18.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33057_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 33057_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 11:31:48.21 -06:41:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 0.882 3593202114082253184 172.95077872607 -06.69011432423 14.5012 13.9362 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.882#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 33070_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 33070_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 11:33:52.15 -09:10:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 0.455 3590204364348549504 173.46741724453 -09.16827396287 14.6306 14.0321 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.455#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 33109_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 33109_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 11:29:22.13 -09:35:30.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33115_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 33115_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 11:32:39.63 -14:13:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 0.917 3561090395958286848 173.16500810686 -14.22892267672 14.5189 14.0465 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.917#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 33139_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 33139_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 11:33:00.48 -14:13:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33155_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 33155_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 11:37:55.32 -14:25:34.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33170_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 33170_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 11:40:26.96 -12:31:43.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33210_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 33210_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 11:33:32.33 -08:32:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 1.017 3591975986818444032 173.38485938454 -08.54160102953 14.5994 14.0762 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.017#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 33243_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 33243_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks
**** FOUND 11:32:20.44 -08:40:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 0.699 3590473847776717056 173.08514632893 -08.66808199779 14.7860 14.2519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.699#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 33338_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129
The candidate 33338_fd_Vir-10-Q1b1x1_2026-04-23_01-51-26_20.00sec_-4.90C_LIGHTs_0129 did not pass the final checks