This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ
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 06 01.3084 2461192.8084 11.44 15:29:59.13 -08:50:39.6
355.42379 37.38191 galactic Lib Second-epoch detections are separated by 0.7" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.92 Undina 3 -1 3 11.5 -0 0
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:29:59.13 -08:50:39.6: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:29:59.13 -08:50:39.6: 15.85 +/- 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,2461192.8084,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260601.3084 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 01.3084 2461192.8084 11.87 15:50:13.62 -13:27:53.6
355.55975 30.60177 galactic Lib Second-epoch detections are separated by 0.6" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.346 Hermentaria 2 -1 3 11.6 -0 0
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:50:13.62 -13:27:53.6: 15.48 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:50:13.62 -13:27:53.6: 15.39 +/- 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,2461192.8084,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260601.3084 11.87CV 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
Mean magnitude and position on the discovery images:
2026 06 01.3084 2461192.8084 12.43 15:18:10.45 -07:52:42.9
353.63987 40.12656 galactic Lib Second-epoch detections are separated by 0.1" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.269 Justitia 3 -1 3 12.3 0 0
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:18:10.45 -07:52:42.9: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:18:10.45 -07:52:42.9: 15.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461192.8084,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260601.3084 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 01.3084 2461192.8084 12.51 15:32:27.40 -09:09:04.4
355.68219 36.73077 galactic Lib Second-epoch detections are separated by 0.6" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.776 Berbericia 2 -1 3 12.6 0 -0
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:32:27.40 -09:09:04.4: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:32:27.40 -09:09:04.4: 15.81 +/- 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,2461192.8084,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260601.3084 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 01.3084 2461192.8084 13.11 15:41:32.15 -13:21:26.6
353.92969 32.19646 galactic Lib Second-epoch detections are separated by 0.8" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.563 Suleika 2 -1 2 13.3 -0 0
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:41:32.15 -13:21:26.6: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:41:32.15 -13:21:26.6: 15.62 +/- 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,2461192.8084,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260601.3084 13.11CV 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: 2461153.89842042 23.04.2026 09:33:33.524 /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
First image: 2461153.89842042 23.04.2026 09:33:33.524 /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
Last image: 2461192.80870563 01.06.2026 07:24:22.166 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 0
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.67
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 2 seconds
Number of parallel threads: 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): 5889
Objects passed selection criteria: 5873
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 4514.5
Average stars matched: 4374.25 (96.8933 %)
Memory usage VmPeak: 112632 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 31 16:54:47 CDT 2026
VaST build number 1.0rc89-84-gccae57d3
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-31)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jun 1 02:26:55 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461153.89842042 23.04.2026 09:33:33.524 /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
First image: 2461153.89842042 23.04.2026 09:33:33.524 /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
Last image: 2461192.80870563 01.06.2026 07:24:22.166 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 12
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.36
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: 17 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): 39564
Objects passed selection criteria: 39486
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 31757
Average stars matched: 30846 (97.1313 %)
Memory usage VmPeak: 145980 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 31 16:54:47 CDT 2026
VaST build number 1.0rc89-84-gccae57d3
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-31)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jun 1 02:28:33 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
SExtractor catalog cache: saved Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat to cache
SExtractor catalog cache: saved Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.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/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.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: 2461192.80818927
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_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits exists and is non-empty
Saving wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits to local_wcs_cache/
'wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits' -> 'local_wcs_cache/wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits'
wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits exists and is non-empty
Saving wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits to local_wcs_cache/
'wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits' -> 'local_wcs_cache/wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits'
wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits exists and is non-empty
Saving wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits to local_wcs_cache/
'wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits' -> 'local_wcs_cache/wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits'
wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits exists and is non-empty
Saving wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits to local_wcs_cache/
'wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits' -> 'local_wcs_cache/wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits (1st reference image)
verification OK: wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 15:25:43.642 -10:00:07.17 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_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits (1st new image)
verification OK: wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
Image size: 937.0'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:25:44.100 -09:59:45.17 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:25:43.642 -10:00:07.17
Second-epoch image center 15:25:44.100 -09:59:45.17
Angular distance between the image centers 0.0064 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits (2nd new image)
verification OK: wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
Image size: 937.0'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:25:45.844 -10:00:04.44 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 15:25:43.642 -10:00:07.17
Second-epoch image center 15:25:45.844 -10:00:04.44
Angular distance between the image centers 0.0091 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 15:25:44.100 -09:59:45.17
Second-epoch second image center 15:25:45.844 -10:00:04.44
Angular distance between the image centers 0.00894 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/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits &> /tmp/tmp.8zCdUoN3mZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits &> /tmp/tmp.XZFFVMY5Qk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits &> /tmp/tmp.BQRWA75hWb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits &> /tmp/tmp.qdrQjLhqCF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.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_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits and wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits and wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat
Found non-empty wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits and wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat
The reference image (wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits) and catalog (wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat) found
'wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat' -> 'wcsmag.cat'
Read 8132 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 222.9892 to 239.6626 deg, Dec -15.6642 to -4.1937 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 222.9892 to 239.6626 deg, Dec -15.6642 to -4.1937 deg
Loaded 6002 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): 4551 out of 4710 total matches.
Matched with Tycho-2 4710 out of 8132 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.736000
a=0.000000 b=1.000000 c=22.736000
From vast_summary.log: estimated ref. image limiting mag.: -7.67
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.07
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.07
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 8132 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 222.9892 to 239.6626 deg, Dec -15.6642 to -4.1937 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 222.9892 to 239.6626 deg, Dec -15.6642 to -4.1937 deg
Loaded 6002 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): 4551 out of 4710 total matches.
Matched with Tycho-2 4710 out of 8132 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits:
Forced-photometry filter: calibrated wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits -> calib.txt_param_ref_wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits (aperture=5.9)
Read 8122 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 223.3808 to 239.4992 deg, Dec -15.2688 to -4.7095 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 223.3808 to 239.4992 deg, Dec -15.2688 to -4.7095 deg
Loaded 5366 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): 4509 out of 4666 total matches.
Matched with Tycho-2 4666 out of 8122 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits:
Forced-photometry filter: calibrated wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits -> calib.txt_param_ref_wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
2.2 pix Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
2.4 pix fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
2.3 pix fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
2.2 pix wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
2.2 pix wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
Limiting magnitude estimates:
15.1 mag. Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
15.0 mag. Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
13.8 mag. fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
13.9 mag. fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 11.0 (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.8zCdUoN3mZ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits' -> 'wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
WCS_IMAGE_NAME=wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
WCS-calibrated image found: wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
Checking if the catalog wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat corresponding to the image wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits alredy exist and is non-empty...
Catalog wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat corresponding to the image wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
WCS catalog name: wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=500, passed=8132
Got 8132 stars (including 7623 good ones) from the SExtractor catalog wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat
util/solve_plate_with_UCAC5 got 8132 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 7988 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 7988 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 7988 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits N_match=967 sigma_overall_arcsec=0.261 sigma_q1_arcsec=0.252 sigma_q2_arcsec=0.351 sigma_q3_arcsec=0.225 sigma_q4_arcsec=0.221 n_q1=252 n_q2=185 n_q3=262 n_q4=268 worst_quadrant_to_overall_ratio=1.342
The image catalog is written to wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits -region wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.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.XZFFVMY5Qk (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_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits' -> 'wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
WCS_IMAGE_NAME=wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
WCS-calibrated image found: wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
Checking if the catalog wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.cat corresponding to the image wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits alredy exist and is non-empty...
Catalog wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.cat corresponding to the image wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
WCS catalog name: wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=502, passed=8122
Got 8122 stars (including 7614 good ones) from the SExtractor catalog wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.cat
util/solve_plate_with_UCAC5 got 8122 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 8023 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 8023 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 8023 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits N_match=968 sigma_overall_arcsec=0.444 sigma_q1_arcsec=0.319 sigma_q2_arcsec=0.609 sigma_q3_arcsec=0.340 sigma_q4_arcsec=0.538 n_q1=226 n_q2=215 n_q3=242 n_q4=285 worst_quadrant_to_overall_ratio=1.371
The image catalog is written to wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits -region wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.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.BQRWA75hWb (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
WCS_IMAGE_NAME=wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
WCS-calibrated image found: wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
Checking if the catalog wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits.cat corresponding to the image wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits.cat corresponding to the image wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
WCS catalog name: wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=269, passed=3375
Got 3375 stars (including 3104 good ones) from the SExtractor catalog wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits.cat
util/solve_plate_with_UCAC5 got 3375 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 3329 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 3331 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 3331 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits N_match=967 sigma_overall_arcsec=0.476 sigma_q1_arcsec=0.367 sigma_q2_arcsec=0.724 sigma_q3_arcsec=0.406 sigma_q4_arcsec=0.596 n_q1=230 n_q2=212 n_q3=236 n_q4=289 worst_quadrant_to_overall_ratio=1.521
The image catalog is written to wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits -region wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.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.qdrQjLhqCF (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
WCS_IMAGE_NAME=wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
WCS-calibrated image found: wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
Checking if the catalog wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits.cat corresponding to the image wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits.cat corresponding to the image wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
WCS catalog name: wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=307, passed=3326
Got 3326 stars (including 3016 good ones) from the SExtractor catalog wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits.cat
util/solve_plate_with_UCAC5 got 3326 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 3295 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 3295 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 3295 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits N_match=967 sigma_overall_arcsec=0.482 sigma_q1_arcsec=0.380 sigma_q2_arcsec=0.638 sigma_q3_arcsec=0.423 sigma_q4_arcsec=0.586 n_q1=236 n_q2=214 n_q3=233 n_q4=284 worst_quadrant_to_overall_ratio=1.324
The image catalog is written to wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits -region wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits sigma_overall=0.261 worst_q_ratio=1.342
ref2=Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits sigma_overall=0.444 worst_q_ratio=1.371
new1=fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits sigma_overall=0.476 worst_q_ratio=1.521
new2=fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits sigma_overall=0.482 worst_q_ratio=1.324
reference average sigma_overall=0.3525 worst_q_ratio=1.3565
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258_astrometric_residuals.png (967 matched stars from wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275_astrometric_residuals.png (968 matched stars from wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002_astrometric_residuals.png (967 matched stars from wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003_astrometric_residuals.png (967 matched stars from wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits'
Saving fully-calibrated image wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits'
Preparing the HTML report for the field Lib-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Lib-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
SExtractor catalog cache: saved Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat to cache
SExtractor catalog cache: saved Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
Creating symlink local_wcs_cache/wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.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_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits exists and is non-empty
wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits exists and is non-empty
wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits exists and is non-empty
wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits (1st reference image)
verification OK: wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 15:25:43.642 -10:00:07.17 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_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits (1st new image)
verification OK: wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
Image size: 937.0'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:25:44.100 -09:59:45.17 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:25:43.642 -10:00:07.17
Second-epoch image center 15:25:44.100 -09:59:45.17
Angular distance between the image centers 0.0064 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits (2nd new image)
verification OK: wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
Image size: 937.0'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:25:45.844 -10:00:04.44 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 15:25:43.642 -10:00:07.17
Second-epoch image center 15:25:45.844 -10:00:04.44
Angular distance between the image centers 0.0091 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 15:25:44.100 -09:59:45.17
Second-epoch second image center 15:25:45.844 -10:00:04.44
Angular distance between the image centers 0.00894 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/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits &> /tmp/tmp.z2PdGz5MFr
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits &> /tmp/tmp.wfYcgplQlC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits &> /tmp/tmp.ST954zieg2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits &> /tmp/tmp.QaxJi0XnSg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.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_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits and wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits and wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat
Found non-empty wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits and wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat
The reference image (wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits) and catalog (wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat) found
'wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat' -> 'wcsmag.cat'
Read 56059 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 222.9892 to 239.6626 deg, Dec -15.6809 to -4.1523 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 222.9892 to 239.6626 deg, Dec -15.6809 to -4.1523 deg
Loaded 6037 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): 4376 out of 4830 total matches.
Matched with Tycho-2 4830 out of 56059 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.606950
a=0.000000 b=1.000000 c=22.606950
From vast_summary.log: estimated ref. image limiting mag.: -7.36
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.25
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.25
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 56059 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 222.9892 to 239.6626 deg, Dec -15.6809 to -4.1523 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 222.9892 to 239.6626 deg, Dec -15.6809 to -4.1523 deg
Loaded 6037 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): 4376 out of 4830 total matches.
Matched with Tycho-2 4830 out of 56059 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits:
Forced-photometry filter: calibrated wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits -> calib.txt_param_ref_wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits (aperture=4.5)
Read 50094 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 223.3438 to 239.5045 deg, Dec -15.2716 to -4.7095 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 223.3438 to 239.5045 deg, Dec -15.2716 to -4.7095 deg
Loaded 5381 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): 4369 out of 4768 total matches.
Matched with Tycho-2 4768 out of 50094 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits:
Forced-photometry filter: calibrated wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits -> calib.txt_param_ref_wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 8 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
2.1 pix Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
2.3 pix fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
2.2 pix fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
2.0 pix wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
2.1 pix wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
Limiting magnitude estimates:
15.2 mag. Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
15.2 mag. Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
14.0 mag. fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
14.0 mag. fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.5 (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.z2PdGz5MFr (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits' -> 'wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
WCS_IMAGE_NAME=wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
WCS-calibrated image found: wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
Checking if the catalog wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat corresponding to the image wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits alredy exist and is non-empty...
Catalog wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat corresponding to the image wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
WCS catalog name: wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=2373, passed=56051
Got 56051 stars (including 53576 good ones) from the SExtractor catalog wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat
util/solve_plate_with_UCAC5 got 56051 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.7 to -4.2)
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(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 55262 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 431 (Dec -15.7 to -4.2)
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(), 55261 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 55261 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! :)
WCS_QUALITY_DIAG: file=Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits N_match=971 sigma_overall_arcsec=0.261 sigma_q1_arcsec=0.241 sigma_q2_arcsec=0.349 sigma_q3_arcsec=0.216 sigma_q4_arcsec=0.252 n_q1=258 n_q2=191 n_q3=251 n_q4=271 worst_quadrant_to_overall_ratio=1.341
The image catalog is written to wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits -region wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.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.wfYcgplQlC (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_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits' -> 'wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
WCS_IMAGE_NAME=wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
WCS-calibrated image found: wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
Checking if the catalog wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.cat corresponding to the image wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits alredy exist and is non-empty...
Catalog wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.cat corresponding to the image wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
WCS catalog name: wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=2552, passed=50088
Got 50088 stars (including 47468 good ones) from the SExtractor catalog wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.cat
util/solve_plate_with_UCAC5 got 50088 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 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(), 965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 49374 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 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(), 49371 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 49371 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits N_match=972 sigma_overall_arcsec=0.453 sigma_q1_arcsec=0.319 sigma_q2_arcsec=0.593 sigma_q3_arcsec=0.343 sigma_q4_arcsec=0.577 n_q1=252 n_q2=202 n_q3=251 n_q4=267 worst_quadrant_to_overall_ratio=1.309
The image catalog is written to wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits -region wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.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.ST954zieg2 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
WCS_IMAGE_NAME=wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
WCS-calibrated image found: wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
Checking if the catalog wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits.cat corresponding to the image wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits.cat corresponding to the image wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
WCS catalog name: wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=934, passed=21924
Got 21924 stars (including 20960 good ones) from the SExtractor catalog wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits.cat
util/solve_plate_with_UCAC5 got 21924 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 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: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 21690 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 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(), 21689 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 21689 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits N_match=972 sigma_overall_arcsec=0.474 sigma_q1_arcsec=0.392 sigma_q2_arcsec=0.674 sigma_q3_arcsec=0.393 sigma_q4_arcsec=0.572 n_q1=258 n_q2=198 n_q3=251 n_q4=265 worst_quadrant_to_overall_ratio=1.422
The image catalog is written to wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits -region wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.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.QaxJi0XnSg (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
WCS_IMAGE_NAME=wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
WCS-calibrated image found: wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
Checking if the catalog wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits.cat corresponding to the image wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits.cat corresponding to the image wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
WCS catalog name: wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=1026, passed=22692
Got 22692 stars (including 21627 good ones) from the SExtractor catalog wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits.cat
util/solve_plate_with_UCAC5 got 22692 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 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: 969 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 22350 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 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: 969 matched stars entering correct_measured_positions(), 22349 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 22349 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits N_match=969 sigma_overall_arcsec=0.476 sigma_q1_arcsec=0.394 sigma_q2_arcsec=0.657 sigma_q3_arcsec=0.436 sigma_q4_arcsec=0.553 n_q1=263 n_q2=196 n_q3=247 n_q4=263 worst_quadrant_to_overall_ratio=1.380
The image catalog is written to wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits -region wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-23-37_20.00sec_4.90C_LIGHT_0002.fits
Saving fully-calibrated image wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Lib-02-Q2b1x1_022459_TTUQ2b1x1_2746265_od5njJqZ/wcs_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003.fits
Preparing the HTML report for the field Lib-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:29:59.13 -08:50:39.6: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:32:27.40 -09:09:04.4: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:18:17.84 -10:08:30.2: 13.22 +/- 0.03 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:18:10.45 -07:52:42.9: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:48:28.54 -13:00:59.3: 12.65 +/- 0.02 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:50:13.62 -13:27:53.6: 15.48 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:41:32.15 -13:21:26.6: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:50:13.62 -13:27:53.6: 15.39 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:29:59.13 -08:50:39.6: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:48:28.54 -13:00:59.3: 12.65 +/- 0.03 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:18:17.84 -10:08:30.2: 13.19 +/- 0.04 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:32:27.40 -09:09:04.4: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:18:10.45 -07:52:42.9: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:41:32.15 -13:21:26.6: 15.62 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.21 +/- 0.03
Forced photometry reference-image weighted average: 12.65 +/- 0.02
Forced photometry filter REJECTED candidate at 15:18:17.84 -10:08:30.2: ref_mag=13.21 +/- 0.03 new_mean_mag=13.1162 delta=0.09 (need > 0.90)
Forced photometry filter REJECTED candidate at 15:48:28.54 -13:00:59.3: ref_mag=12.65 +/- 0.02 new_mean_mag=12.8953 delta=-0.25 (need > 0.90)
Adding exclusion_list_local.txt__out69586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69594.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69601.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69602.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69628.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 69574_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003
The candidate 69574_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003 did not pass the final checks
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Considering the candidate 69586_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003
Preparing report for the candidate 69586_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003
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Considering the candidate 69594_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003
Preparing report for the candidate 69594_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003
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Considering the candidate 69601_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003
Preparing report for the candidate 69601_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003
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Considering the candidate 69602_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003
Preparing report for the candidate 69602_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003
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Considering the candidate 69628_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003
Preparing report for the candidate 69628_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003
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Considering the candidate 69629_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003
The candidate 69629_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003 did not pass the final checks
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Considering the candidate 69642_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003
The candidate 69642_fd_Lib-02-Q2b1x1_2026-06-01_02-24-22_20.00sec_4.90C_LIGHT_0003 did not pass the final checks