This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF
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
VARIABLE_NAME,2461147.8031,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.3031 11.74CV 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,2461147.8031,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.3031 13.06CV 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!
TCP 2026 04 17.3031* 14 08 10.61 -09 41 41.9 13.3 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.8031,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.3031 13.34CV 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!
TCP 2026 04 17.3031* 14 10 36.08 -08 55 31.2 14.0 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.8031,14.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.3031 14.02CV 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!
TCP 2026 04 17.3031* 14 09 26.30 -07 03 09.1 14.2 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.8031,14.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.3031 14.16CV 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!
TCP 2026 04 17.3031* 14 42 00.60 -05 49 58.0 11.3 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
XY Vir,2461147.8031,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
XY Vir 20260417.3031 11.31CV 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: 2461098.90985984 27.02.2026 09:50:01.890 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
First image: 2461098.90985984 27.02.2026 09:50:01.890 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Last image: 2461147.80412186 17.04.2026 07:17:46.129 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.16
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 4928
Objects passed selection criteria: 4923
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 4721.25
Average stars matched: 4508.75 (95.4991 %)
Memory usage VmPeak: 111312 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 17 02:23:42 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: 2461098.90985984 27.02.2026 09:50:01.890 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
First image: 2461098.90985984 27.02.2026 09:50:01.890 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Last image: 2461147.80412186 17.04.2026 07:17:46.129 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 71
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.87
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): 29073
Objects passed selection criteria: 29032
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 27863.8
Average stars matched: 26410.5 (94.7844 %)
Memory usage VmPeak: 132224 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 17 02:24:35 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
SExtractor catalog cache: saved Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat to cache
SExtractor catalog cache: saved Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.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-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.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: 2461147.80201215
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits exists and is non-empty
Saving wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits to local_wcs_cache/
'wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits' -> 'local_wcs_cache/wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits'
wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits exists and is non-empty
Saving wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits to local_wcs_cache/
'wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits' -> 'local_wcs_cache/wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits'
wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits exists and is non-empty
Saving wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits to local_wcs_cache/
'wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits' -> 'local_wcs_cache/wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits'
wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits exists and is non-empty
Saving wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits to local_wcs_cache/
'wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits' -> 'local_wcs_cache/wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits (1st reference image)
verification OK: wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Image size: 937.3'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 14:34:25.896 -10:01:24.58 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits (1st new image)
verification OK: wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits
Image size: 937.0'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 14:33:58.328 -09:59:31.34 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:34:25.896 -10:01:24.58
Second-epoch image center 14:33:58.328 -09:59:31.34
Angular distance between the image centers 0.1174 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits (2nd new image)
verification OK: wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
Image size: 936.9'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 14:34:00.304 -09:59:55.61 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 14:34:25.896 -10:01:24.58
Second-epoch image center 14:34:00.304 -09:59:55.61
Angular distance between the image centers 0.1079 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 14:33:58.328 -09:59:31.34
Second-epoch second image center 14:34:00.304 -09:59:55.61
Angular distance between the image centers 0.01055 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-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits &> /tmp/tmp.r9ds4yVA5k
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits &> /tmp/tmp.Kroh1FB455
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits &> /tmp/tmp.5IUxSCm3o2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits &> /tmp/tmp.QzET3vHsPI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.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-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits and wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.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-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits and wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
Found non-empty wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits and wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
The reference image (wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits) and catalog (wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat) found
'wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat' -> 'wcsmag.cat'
Read 5992 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 210.5294 to 226.6314 deg, Dec -15.2867 to -4.6831 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 210.5294 to 226.6314 deg, Dec -15.2867 to -4.6831 deg
Loaded 4504 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): 3597 out of 3683 total matches.
Matched with Tycho-2 3683 out of 5992 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.914760
a=0.000000 b=1.000000 c=22.914760
From vast_summary.log: estimated ref. image limiting mag.: -8.16
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.75
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.75
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.5 pix Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
2.4 pix Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
2.7 pix fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits
3.0 pix fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
Limiting magnitude estimates:
14.8 mag. Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
14.8 mag. Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
14.8 mag. fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits
14.8 mag. fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 11.9 (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.r9ds4yVA5k (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits 567.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.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-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits' -> 'wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
WCS_IMAGE_NAME=wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
WCS-calibrated image found: wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Checking if the catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits alredy exist and is non-empty...
Catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
WCS catalog name: wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=377, passed=5992
Got 5992 stars (including 5611 good ones) from the SExtractor catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
util/solve_plate_with_UCAC5 got 5992 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 5896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 5898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 5899 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 971 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_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits -region wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.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.Kroh1FB455 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits 567.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.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-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits' -> 'wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
WCS_IMAGE_NAME=wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
WCS-calibrated image found: wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
Checking if the catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits alredy exist and is non-empty...
Catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
WCS catalog name: wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=404, passed=5931
Got 5931 stars (including 5520 good ones) from the SExtractor catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat
util/solve_plate_with_UCAC5 got 5931 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 5841 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 973 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(), 5841 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 5841 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits -region wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.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.5IUxSCm3o2 (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_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.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_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits
WCS_IMAGE_NAME=wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits
WCS-calibrated image found: wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits
Checking if the catalog wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits
WCS catalog name: wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=456, passed=6515
Got 6515 stars (including 6057 good ones) from the SExtractor catalog wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits.cat
util/solve_plate_with_UCAC5 got 6515 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
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: 967 matched stars entering correct_measured_positions(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 6342 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
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: 967 matched stars entering correct_measured_positions(), 6343 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 6343 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits -region wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.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.QzET3vHsPI (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_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.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_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
WCS_IMAGE_NAME=wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
WCS-calibrated image found: wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
Checking if the catalog wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
WCS catalog name: wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=485, passed=6441
Got 6441 stars (including 5954 good ones) from the SExtractor catalog wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits.cat
util/solve_plate_with_UCAC5 got 6441 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 6277 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 6279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 6279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
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_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits -region wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.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-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits'
Saving fully-calibrated image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits'
Saving fully-calibrated image wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits'
Saving fully-calibrated image wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits'
Preparing the HTML report for the field Lib-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20220.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20246.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: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20193_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 20193_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:10:21.50 -13:18:14.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20210_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 20210_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:15:44.62 -05:52:10.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20220_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 20220_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:42:00.60 -05:49:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.33, MAG_FAINT_SEARCH_LIMIT=12.31)GAIADR2_OUTPUT=# 0.666 6331703906602883584 220.50261574614 -05.83257726540 11.6139 10.0819 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.666#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20246_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
Preparing report for the candidate 20246_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01128_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 01128_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:28:45.16 -13:28:57.0 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Lib-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
14:23:12.09 -12:44:52.5
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
SExtractor catalog cache: saved Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat to cache
SExtractor catalog cache: saved Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.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-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Creating symlink local_wcs_cache/wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.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-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits exists and is non-empty
wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits exists and is non-empty
wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits exists and is non-empty
wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits (1st reference image)
verification OK: wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Image size: 937.3'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 14:34:25.896 -10:01:24.58 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits (1st new image)
verification OK: wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits
Image size: 937.0'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 14:33:58.328 -09:59:31.34 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:34:25.896 -10:01:24.58
Second-epoch image center 14:33:58.328 -09:59:31.34
Angular distance between the image centers 0.1174 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits (2nd new image)
verification OK: wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
Image size: 936.9'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 14:34:00.304 -09:59:55.61 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 14:34:25.896 -10:01:24.58
Second-epoch image center 14:34:00.304 -09:59:55.61
Angular distance between the image centers 0.1079 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 14:33:58.328 -09:59:31.34
Second-epoch second image center 14:34:00.304 -09:59:55.61
Angular distance between the image centers 0.01055 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-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits &> /tmp/tmp.a9kpKkHrXf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits &> /tmp/tmp.CF5q4TlLxO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits &> /tmp/tmp.a6KBAVOeEp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits &> /tmp/tmp.vQqZ9kV0O5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.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-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits and wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.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-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits and wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
Found non-empty wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits and wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
The reference image (wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits) and catalog (wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat) found
'wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat' -> 'wcsmag.cat'
Read 33758 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 210.4848 to 226.6346 deg, Dec -15.2985 to -4.6504 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 210.4848 to 226.6346 deg, Dec -15.2985 to -4.6504 deg
Loaded 4537 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): 3660 out of 3887 total matches.
Matched with Tycho-2 3887 out of 33758 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.758633
a=0.000000 b=1.000000 c=22.758633
From vast_summary.log: estimated ref. image limiting mag.: -7.87
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.89
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.89
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 35 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
2.3 pix Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
2.4 pix fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits
2.5 pix fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
Limiting magnitude estimates:
14.9 mag. Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
14.9 mag. Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
15.0 mag. fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits
14.9 mag. fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 14.2 (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.a9kpKkHrXf (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits 567.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.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-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits' -> 'wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
WCS_IMAGE_NAME=wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
WCS-calibrated image found: wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Checking if the catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits alredy exist and is non-empty...
Catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
WCS catalog name: wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1364, passed=33749
Got 33749 stars (including 32349 good ones) from the SExtractor catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
util/solve_plate_with_UCAC5 got 33749 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 33427 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 33427 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 33427 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits -region wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.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.CF5q4TlLxO (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits 567.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.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-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits' -> 'wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
WCS_IMAGE_NAME=wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
WCS-calibrated image found: wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
Checking if the catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits alredy exist and is non-empty...
Catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
WCS catalog name: wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1488, passed=34765
Got 34765 stars (including 33244 good ones) from the SExtractor catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat
util/solve_plate_with_UCAC5 got 34765 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 34386 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 34386 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 34386 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits -region wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.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.a6KBAVOeEp (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_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.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_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits
WCS_IMAGE_NAME=wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits
WCS-calibrated image found: wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits
Checking if the catalog wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits
WCS catalog name: wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=2326, passed=35298
Got 35298 stars (including 32927 good ones) from the SExtractor catalog wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits.cat
util/solve_plate_with_UCAC5 got 35298 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 34582 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 34582 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 34582 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits -region wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.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.vQqZ9kV0O5 (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_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.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_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
WCS_IMAGE_NAME=wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
WCS-calibrated image found: wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
Checking if the catalog wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
WCS catalog name: wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=2587, passed=33232
Got 33232 stars (including 30615 good ones) from the SExtractor catalog wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits.cat
util/solve_plate_with_UCAC5 got 33232 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 32386 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 32387 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 32386 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits -region wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.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-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.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_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Saving fully-calibrated image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.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_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
Saving fully-calibrated image wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.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_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-14-43_20.00sec_-4.90C_LIGHT_0245.fits
Saving fully-calibrated image wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.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_2026-04-17_CI_Lib-01-Q2b1x1_021829_TTUQ2b1x1_3466305_zYCoUxLF/wcs_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246.fits
Preparing the HTML report for the field Lib-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52974.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53058.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53158.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53197.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53202.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53223.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53252.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53270.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53277.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53279.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53333.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53342.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53344.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53352.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out25642.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52947.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52961.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53110.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53167.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
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 52749_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 52749_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:09:07.61 -05:56:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52752_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 52752_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:26:33.27 -07:00:20.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52758_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 52758_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:29:27.74 -12:05:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52817_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 52817_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:23:12.10 -12:44:52.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52947_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
Preparing report for the candidate 52947_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
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Considering the candidate 52961_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
Preparing report for the candidate 52961_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
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Considering the candidate 52974_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 52974_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:23:15.93 -06:31:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 1.021 3641442877513198592 215.81666000392 -06.52484525301 13.3184 12.7948 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.021#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53058_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 53058_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:18:01.16 -07:39:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 3.209 3639756261035933696 214.50564361848 -07.65366453794 14.1683 13.6471 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.209#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53083_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 53083_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:15:54.22 -05:59:05.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 53110_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
Preparing report for the candidate 53110_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
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Considering the candidate 53158_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 53158_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:08:49.63 -12:36:26.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)
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Considering the candidate 53167_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
Preparing report for the candidate 53167_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
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Considering the candidate 53172_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 53172_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:31:12.10 -10:20:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53186_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 53186_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:07:31.33 -10:21:21.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53197_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 53197_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:06:54.89 -12:54:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 0.964 6302485969938205440 211.72851106906 -12.91231344404 14.2781 13.7476 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.964#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53202_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 53202_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:10:02.73 -06:18:00.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.54, MAG_FAINT_SEARCH_LIMIT=15.52)GAIADR2_OUTPUT=# 0.880 3640573095096242048 212.51161244473 -06.30025790146 14.7000 14.1293 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.880#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53207_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 53207_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:10:20.56 -06:28:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 1.309 3640522861158729984 212.58530588454 -06.46955072843 14.5661 14.0257 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.309#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53214_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 53214_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:07:30.37 -11:06:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53215_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 53215_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:11:18.09 -14:16:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53223_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 53223_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:29:40.53 -05:57:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 0.892 3641360689020045824 217.41878569847 -05.95268536099 14.3156 13.4672 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.892#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53252_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 53252_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:19:30.59 -06:34:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 0.434 3639978568543262208 214.87751640893 -06.57189408465 14.2656 13.3384 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.434#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53258_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 53258_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:13:40.97 -08:28:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53270_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 53270_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:17:11.20 -07:45:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 0.712 3639381430650182528 214.29663598396 -07.75833232288 14.3596 13.7313 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.712#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53277_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 53277_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:37:58.32 -11:03:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 3.245 6324864845494699264 219.49390383002 -11.05124404004 14.8084 14.2543 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.245#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53279_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 53279_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:18:14.13 -09:47:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 0.384 6328993580376385536 214.55889464527 -09.78896607232 14.4502 13.9102 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.384#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53317_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 53317_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:50:07.48 -12:40:51.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53330_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 53330_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:42:25.15 -11:15:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 2.342 6324138721143735552 220.60425651076 -11.26278249063 14.4849 13.7866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.342#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53333_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 53333_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:17:04.92 -12:53:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 0.485 6303058574978307584 214.27045104501 -12.89395736051 14.3736 13.7685 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.485#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53342_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 53342_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:36:25.89 -14:13:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 0.856 6323075871356738560 219.10788056438 -14.23132095047 14.3330 13.4712 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.856#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53344_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 53344_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:40:02.97 -12:07:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 0.661 6323930982165701248 220.01249460627 -12.12371938802 14.5517 14.0300 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.661#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53352_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 53352_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:36:05.63 -13:46:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 2.555 6323152287414898176 219.02303621135 -13.76897611949 14.8581 14.2646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.555#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25997_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 25997_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:15:44.64 -05:52:10.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05170_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 05170_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks
**** FOUND 14:10:21.51 -13:18:14.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04974_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246
The candidate 04974_fd_Lib-01-Q2b1x1_2026-04-17_02-17-46_20.00sec_-5.00C_LIGHT_0246 did not pass the final checks