This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J162325-1551.9,2461143.9562,10.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J162325-1551.9 20260413.4562 10.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461143.9562,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.4562 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461143.9562,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.4562 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461143.9562,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.4562 13.43CV 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
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
UU Lib,2461143.9562,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
UU Lib 20260413.4562 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VW Lib,2461143.9562,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VW Lib 20260413.4562 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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
UY Lib,2461143.9562,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
UY Lib 20260413.4562 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.92118531 27.02.2026 10:06:20.411 /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
First image: 2461098.92118531 27.02.2026 10:06:20.411 /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
Last image: 2461143.95656520 13.04.2026 10:57:17.233 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.42
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): 5913
Objects passed selection criteria: 5902
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 4829.25
Average stars matched: 4721.25 (97.7636 %)
Memory usage VmPeak: 111880 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 06:41:29 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.92118531 27.02.2026 10:06:20.411 /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
First image: 2461098.92118531 27.02.2026 10:06:20.411 /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
Last image: 2461143.95656520 13.04.2026 10:57:17.233 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 36
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.11
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 15 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 41686
Objects passed selection criteria: 41632
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 35979.5
Average stars matched: 34506.2 (95.9053 %)
Memory usage VmPeak: 143716 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 06:42:18 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
SExtractor catalog cache: saved Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits.cat to cache
SExtractor catalog cache: saved Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.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-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.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: 2461143.95582515
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits exists and is non-empty
Saving wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits to local_wcs_cache/
'wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits' -> 'local_wcs_cache/wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits'
wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits exists and is non-empty
Saving wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits to local_wcs_cache/
'wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits' -> 'local_wcs_cache/wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits'
wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits exists and is non-empty
Saving wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits to local_wcs_cache/
'wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits' -> 'local_wcs_cache/wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits'
wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits exists and is non-empty
Saving wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits to local_wcs_cache/
'wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits' -> 'local_wcs_cache/wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits'
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:00:00.606 -17:59:38.66
Second-epoch image center 15:59:55.121 -17:56:54.96
Angular distance between the image centers 0.0504 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:00:00.606 -17:59:38.66
Second-epoch image center 15:59:52.892 -17:57:38.60
Angular distance between the image centers 0.0452 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 15:59:55.121 -17:56:54.96
Second-epoch second image center 15:59:52.892 -17:57:38.60
Angular distance between the image centers 0.01500 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-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits &> /tmp/tmp.xPXEbmKn5q
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits &> /tmp/tmp.yutpptNkZc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits &> /tmp/tmp.OFk9HvOfLT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits &> /tmp/tmp.lUa8Nq8i8A
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.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-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits and wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits and wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits.cat
Found non-empty wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits and wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits.cat
The reference image (wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits) and catalog (wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits.cat) found
'wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits.cat' -> 'wcsmag.cat'
Read 6162 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 231.4632 to 248.3943 deg, Dec -23.2674 to -12.5886 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 231.4632 to 248.3943 deg, Dec -23.2674 to -12.5886 deg
Loaded 5955 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): 4295 out of 4400 total matches.
Matched with Tycho-2 4400 out of 6162 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.872392
a=0.000000 b=1.000000 c=22.872392
From vast_summary.log: estimated ref. image limiting mag.: -8.42
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.45
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.45
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
2.4 pix Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits
2.3 pix fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits
2.6 pix fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
Limiting magnitude estimates:
14.5 mag. Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
14.5 mag. Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits
13.4 mag. fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits
13.5 mag. fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
All-image limiting magnitude estimate: 13.4 (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.xPXEbmKn5q (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-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.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_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.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-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.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-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits' -> 'wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
WCS-calibrated image found: wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
Checking if the catalog wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits.cat corresponding to the image wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits.cat corresponding to the image wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
WCS catalog name: wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=373, passed=6162
Got 6162 stars (including 5786 good ones) from the SExtractor catalog wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits.cat
util/solve_plate_with_UCAC5 got 6162 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 6079 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 6077 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 6077 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits -region wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.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.yutpptNkZc (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-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.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_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.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-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.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-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits' -> 'wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits
WCS_IMAGE_NAME=wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits
WCS-calibrated image found: wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits
Checking if the catalog wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits.cat corresponding to the image wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits alredy exist and is non-empty...
Catalog wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits.cat corresponding to the image wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits
WCS catalog name: wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=389, passed=6166
Got 6166 stars (including 5773 good ones) from the SExtractor catalog wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits.cat
util/solve_plate_with_UCAC5 got 6166 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 333 to 389 (Dec -23.3 to -12.6)
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: 968 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 6063 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
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 333 to 389 (Dec -23.3 to -12.6)
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(), 6064 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 6064 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits -region wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.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.OFk9HvOfLT (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits
WCS_IMAGE_NAME=wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits
WCS-calibrated image found: wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits
Checking if the catalog wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits.cat corresponding to the image wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits.cat corresponding to the image wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits
WCS catalog name: wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=169, passed=3363
Got 3363 stars (including 3189 good ones) from the SExtractor catalog wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits.cat
util/solve_plate_with_UCAC5 got 3363 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.5 to -12.1)
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: 971 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 3245 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.5 to -12.1)
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: 971 matched stars entering correct_measured_positions(), 3245 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 3245 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits -region wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.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.lUa8Nq8i8A (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
WCS_IMAGE_NAME=wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
WCS-calibrated image found: wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
Checking if the catalog wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits.cat corresponding to the image wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits.cat corresponding to the image wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
WCS catalog name: wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=162, passed=3720
Got 3720 stars (including 3558 good ones) from the SExtractor catalog wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits.cat
util/solve_plate_with_UCAC5 got 3720 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.5 to -12.1)
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(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 3562 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.5 to -12.1)
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(), 3561 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 3561 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits -region wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits'
Saving fully-calibrated image wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits'
Saving fully-calibrated image wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits'
Saving fully-calibrated image wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits'
Preparing the HTML report for the field Lib-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out04382.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 3s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20383_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 20383_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 16:02:05.88 -18:18:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.06, MAG_FAINT_SEARCH_LIMIT=12.04)GAIADR2_OUTPUT=# 1.386 6247616972464104832 240.52454847561 -18.30253437003 10.3541 8.7084 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.386#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20388_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 20388_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 15:42:02.94 -21:10:49.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02508_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 02508_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 15:31:06.05 -18:56:01.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04382_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
Preparing report for the candidate 04382_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 4s
Prepared the HTML report for the field Lib-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
16:23:24.28 -15:51:58.3
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
SExtractor catalog cache: saved Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits.cat to cache
SExtractor catalog cache: saved Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.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-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
Creating symlink local_wcs_cache/wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.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-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits exists and is non-empty
wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits exists and is non-empty
wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits exists and is non-empty
wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits exists and is non-empty
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:00:00.606 -17:59:38.66
Second-epoch image center 15:59:55.121 -17:56:54.96
Angular distance between the image centers 0.0504 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:00:00.606 -17:59:38.66
Second-epoch image center 15:59:52.892 -17:57:38.60
Angular distance between the image centers 0.0452 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 15:59:55.121 -17:56:54.96
Second-epoch second image center 15:59:52.892 -17:57:38.60
Angular distance between the image centers 0.01500 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-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits &> /tmp/tmp.I8xC9oysuV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits &> /tmp/tmp.vZbqXwdGB2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits &> /tmp/tmp.FtsIXIxU3I
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits &> /tmp/tmp.dSV1HJ3L1a
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.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-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits and wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits and wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits.cat
Found non-empty wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits and wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits.cat
The reference image (wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits) and catalog (wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits.cat) found
'wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits.cat' -> 'wcsmag.cat'
Read 44417 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 231.4632 to 248.3943 deg, Dec -23.2703 to -12.5617 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 231.4632 to 248.3943 deg, Dec -23.2703 to -12.5617 deg
Loaded 5972 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): 4828 out of 5199 total matches.
Matched with Tycho-2 5199 out of 44417 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.688479
a=0.000000 b=1.000000 c=22.688479
From vast_summary.log: estimated ref. image limiting mag.: -8.11
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.58
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.58
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 32 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
2.3 pix Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits
2.2 pix fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits
2.5 pix fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
Limiting magnitude estimates:
14.6 mag. Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
14.6 mag. Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits
13.8 mag. fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits
13.8 mag. fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 13.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.I8xC9oysuV (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-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.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_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.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-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.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-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits' -> 'wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
WCS-calibrated image found: wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
Checking if the catalog wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits.cat corresponding to the image wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits.cat corresponding to the image wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
WCS catalog name: wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1941, passed=44410
Got 44410 stars (including 42424 good ones) from the SExtractor catalog wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits.cat
util/solve_plate_with_UCAC5 got 44410 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 333 to 389 (Dec -23.3 to -12.6)
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: 968 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 43678 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
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 333 to 389 (Dec -23.3 to -12.6)
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(), 43678 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 43678 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits -region wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.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.vZbqXwdGB2 (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-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.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_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.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-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.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-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits' -> 'wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits
WCS_IMAGE_NAME=wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits
WCS-calibrated image found: wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits
Checking if the catalog wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits.cat corresponding to the image wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits alredy exist and is non-empty...
Catalog wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits.cat corresponding to the image wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits
WCS catalog name: wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=2017, passed=45530
Got 45530 stars (including 43466 good ones) from the SExtractor catalog wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits.cat
util/solve_plate_with_UCAC5 got 45530 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 967 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(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 44652 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 967 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(), 44652 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 44652 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits -region wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.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.FtsIXIxU3I (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits
WCS_IMAGE_NAME=wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits
WCS-calibrated image found: wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits
Checking if the catalog wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits.cat corresponding to the image wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits.cat corresponding to the image wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits
WCS catalog name: wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=894, passed=28106
Got 28106 stars (including 27177 good ones) from the SExtractor catalog wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits.cat
util/solve_plate_with_UCAC5 got 28106 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.5 to -12.0)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 27291 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.5 to -12.0)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 27292 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 27292 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits -region wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.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.dSV1HJ3L1a (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
WCS_IMAGE_NAME=wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
WCS-calibrated image found: wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
Checking if the catalog wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits.cat corresponding to the image wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits.cat corresponding to the image wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
WCS catalog name: wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1060, passed=27124
Got 27124 stars (including 26030 good ones) from the SExtractor catalog wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits.cat
util/solve_plate_with_UCAC5 got 27124 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.5 to -12.1)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 26196 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.5 to -12.1)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 26197 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 26197 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits -region wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/wcs_Lib-04-Q1b1x1_2026-02-27_04-06-20_20.00sec_-15.00C_LIGHT_0227.fits
Saving fully-calibrated image wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/wcs_Lib-04-Q1b1x1_2026-02-27_04-07-06_20.00sec_-14.90C_LIGHT_0228.fits
Saving fully-calibrated image wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-56-13_20.00sec_-4.90C_LIGHTs_0225.fits
Saving fully-calibrated image wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-04-Q1b1x1_055814_TTUQ1b1x1_11241_VQmd5oSm/wcs_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226.fits
Preparing the HTML report for the field Lib-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out54636.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54639.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54643.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54646.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54647.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54649.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54655.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54674.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54856.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54934.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54989.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55139.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55270.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55277.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55384.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55431.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55443.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55451.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out19431.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22314.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43028.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54784.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55353.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
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 54636_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 54636_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 16:06:42.46 -16:41:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 2.681 6250452956546191744 241.67727176401 -16.68269872625 13.9063 13.2571 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.681#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54639_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 54639_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 15:38:49.64 -14:34:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 1.981 6265396109845043328 234.70729917718 -14.57457320524 13.6768 12.9817 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.981#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54643_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 54643_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 16:32:12.55 -15:05:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 0.687 4325614361559233792 248.05235977070 -15.08718207164 12.5986 12.1219 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.687#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54645_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 54645_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 16:23:01.74 -21:14:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54646_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 54646_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 16:30:19.40 -15:38:20.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)
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Considering the candidate 54647_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 54647_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 15:58:34.68 -19:00:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 0.494 6247474585708294528 239.64464298245 -19.01194073102 12.6174 11.7749 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.494#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54649_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 54649_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 16:25:23.10 -20:25:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 2.063 6244816099729217920 246.34661463479 -20.42326228679 12.2573 11.5137 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.063#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54655_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 54655_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 16:11:33.89 -20:50:06.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 2.197 6243861659216521856 242.89119323054 -20.83447331585 11.5480 10.8556 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.197#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54674_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 54674_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 16:12:05.88 -23:14:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.11, MAG_FAINT_SEARCH_LIMIT=11.09)GAIADR2_OUTPUT=# 0.573 6242180368499938816 243.02464895964 -23.24583542585 9.1656 8.7365 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.573#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54679_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 54679_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 15:47:55.12 -12:41:46.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54784_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
Preparing report for the candidate 54784_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
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Considering the candidate 54856_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 54856_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 16:18:14.70 -23:08:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 5.009 6050451276059051136 244.55976681239 -23.14697033939 11.3039 10.4017 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.009#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54934_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 54934_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 16:31:35.22 -17:43:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 1.506 4323916754263443328 247.89639555299 -17.72235808068 12.1225 11.4388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.506#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54956_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
Preparing report for the candidate 54956_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
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Considering the candidate 54989_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 54989_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 16:18:39.79 -21:48:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 0.081 6244248721669495808 244.66578109515 -21.80214641148 11.9076 11.1198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.081#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55013_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 55013_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 15:37:47.94 -16:09:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55139_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 55139_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 15:41:59.23 -15:33:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 1.262 6262084621338471424 235.49652188755 -15.55745938640 13.3110 12.7320 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.262#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55270_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 55270_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 16:31:17.92 -23:03:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 4.128 6050831535282402048 247.82563185904 -23.05830883363 12.4513 11.5557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.128#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55277_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 55277_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 16:31:50.67 -18:11:15.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 1.929 4323681733652995456 247.96126301208 -18.18714723295 13.1426 12.5191 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.929#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55353_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
Preparing report for the candidate 55353_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
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Considering the candidate 55384_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 55384_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 15:30:01.51 -17:45:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 1.608 6258352638358154112 232.50607720996 -17.75567511739 14.2182 13.4503 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.608#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55431_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 55431_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 15:28:28.81 -18:33:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 2.101 6254915358851272704 232.12059234580 -18.55206624008 14.1470 13.5717 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.101#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55443_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 55443_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 15:32:03.82 -17:34:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 1.517 6255450236897442432 233.01575161175 -17.57638691270 14.3966 13.7318 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.517#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55451_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 55451_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 15:46:01.31 -17:31:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 1.576 6260482804695668480 236.50546911681 -17.52270119931 14.1966 13.4716 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.576#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 19431_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
Preparing report for the candidate 19431_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
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Considering the candidate 01167_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 01167_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 16:17:40.37 -22:53:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03006_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 03006_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 16:26:39.18 -22:18:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 43028_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
Preparing report for the candidate 43028_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
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Considering the candidate 39467_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 39467_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 16:21:32.05 -15:12:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07237_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 07237_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 15:42:03.16 -21:10:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22314_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
Preparing report for the candidate 22314_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
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Considering the candidate 42091_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226
The candidate 42091_fd_Lib-04-Q1b1x1_2026-04-13_05-57-17_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks