This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq
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,2461146.7983,11.25,0.05,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 20260416.2983 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461146.7983,11.63,0.05,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 20260416.2983 11.63CV 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,2461146.7983,12.05,0.05,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 20260416.2983 12.05CV 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,2461146.7983,12.57,0.05,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 20260416.2983 12.57CV 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,2461146.7983,14.21,0.05,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 20260416.2983 14.21CV 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
ATO J228.4509-15.4639,2461146.7983,14.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J228.4509-15.4639 20260416.2983 14.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.92002373 27.02.2026 10:04:40.050 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
First image: 2461098.92002373 27.02.2026 10:04:40.050 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Last image: 2461146.79863317 16.04.2026 07:09:51.906 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.28
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): 5959
Objects passed selection criteria: 5955
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 5520.5
Average stars matched: 5175.5 (93.7506 %)
Memory usage VmPeak: 112096 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 16 02:12:02 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: 2461098.92002373 27.02.2026 10:04:40.050 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
First image: 2461098.92002373 27.02.2026 10:04:40.050 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Last image: 2461146.79863317 16.04.2026 07:09:51.906 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 77
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.97
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: 16 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): 35469
Objects passed selection criteria: 35416
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: 33833.5
Average stars matched: 32339.5 (95.5843 %)
Memory usage VmPeak: 137856 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 16 02:13:11 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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
SExtractor catalog cache: saved Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat to cache
SExtractor catalog cache: saved Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.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: 2461146.79798197
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits exists and is non-empty
Saving wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits to local_wcs_cache/
'wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits' -> 'local_wcs_cache/wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits'
wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits exists and is non-empty
Saving wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits to local_wcs_cache/
'wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits' -> 'local_wcs_cache/wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits'
wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits exists and is non-empty
Saving wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits to local_wcs_cache/
'wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits' -> 'local_wcs_cache/wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits'
wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits exists and is non-empty
Saving wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits to local_wcs_cache/
'wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits' -> 'local_wcs_cache/wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits (1st reference image)
verification OK: wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Image size: 937.4'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 15:07:04.132 -18:01:06.94 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"
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# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits (1st new image)
verification OK: wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits
Image size: 937.1'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:06:34.485 -18:00:29.85 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:07:04.132 -18:01:06.94
Second-epoch image center 15:06:34.485 -18:00:29.85
Angular distance between the image centers 0.1179 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits (2nd new image)
verification OK: wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
Image size: 937.0'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:06:37.221 -18:00:59.25 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 15:07:04.132 -18:01:06.94
Second-epoch image center 15:06:37.221 -18:00:59.25
Angular distance between the image centers 0.1067 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 15:06:34.485 -18:00:29.85
Second-epoch second image center 15:06:37.221 -18:00:59.25
Angular distance between the image centers 0.01357 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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits &> /tmp/tmp.poBOd5Rrp2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits &> /tmp/tmp.TDNAUoeVkW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits &> /tmp/tmp.dygHFcJxz0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits &> /tmp/tmp.1pya0lweVd
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
Found non-empty wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
The reference image (wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits) and catalog (wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat) found
'wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat' -> 'wcsmag.cat'
Read 6705 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 218.3309 to 235.1834 deg, Dec -23.2849 to -12.5918 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 218.3309 to 235.1834 deg, Dec -23.2849 to -12.5918 deg
Loaded 6143 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): 4648 out of 4760 total matches.
Matched with Tycho-2 4760 out of 6705 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.861505
a=0.000000 b=1.000000 c=22.861505
From vast_summary.log: estimated ref. image limiting mag.: -8.28
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.58
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.58
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
2.4 pix Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
3.2 pix fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits
3.2 pix fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
Limiting magnitude estimates:
14.6 mag. Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
14.6 mag. Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
14.6 mag. fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits
14.6 mag. fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 11.7 (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.poBOd5Rrp2 (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_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits' -> 'wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS_IMAGE_NAME=wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS-calibrated image found: wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Checking if the catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits alredy exist and is non-empty...
Catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS catalog name: wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=403, passed=6705
Got 6705 stars (including 6294 good ones) from the SExtractor catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
util/solve_plate_with_UCAC5 got 6705 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6630 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6630 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6630 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits -region wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.TDNAUoeVkW (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_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits' -> 'wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS_IMAGE_NAME=wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS-calibrated image found: wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Checking if the catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits alredy exist and is non-empty...
Catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS catalog name: wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=425, passed=6649
Got 6649 stars (including 6218 good ones) from the SExtractor catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat
util/solve_plate_with_UCAC5 got 6649 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6582 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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6580 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6580 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits -region wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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.dygHFcJxz0 (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_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.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_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits
WCS_IMAGE_NAME=wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits
WCS-calibrated image found: wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits
Checking if the catalog wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits
WCS catalog name: wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=601, passed=7670
Got 7670 stars (including 7064 good ones) from the SExtractor catalog wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits.cat
util/solve_plate_with_UCAC5 got 7670 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 7600 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 7599 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 7599 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits -region wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.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.1pya0lweVd (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_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.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_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
WCS_IMAGE_NAME=wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
WCS-calibrated image found: wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
Checking if the catalog wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
WCS catalog name: wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=602, passed=7663
Got 7663 stars (including 7059 good ones) from the SExtractor catalog wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits.cat
util/solve_plate_with_UCAC5 got 7663 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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 7587 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 7587 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 7587 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits -region wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits'
Saving fully-calibrated image wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits'
Saving fully-calibrated image wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits'
Saving fully-calibrated image wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits'
Preparing the HTML report for the field Lib-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20320.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 20252_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 20252_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 15:17:57.89 -13:57:48.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20295_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 20295_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20320_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 20320_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20325_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 20325_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:47:20.45 -18:29:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.68, MAG_FAINT_SEARCH_LIMIT=12.66)GAIADR2_OUTPUT=# 0.959 6282275292656488960 221.83503562169 -18.49687336045 11.8029 11.1186 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.959#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20335_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 20335_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 15:13:35.86 -14:47:10.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01970_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 01970_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:42:46.41 -20:12:36.3 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-03-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 ####
14:59:21.59 -14:27:58.3
15:11:42.82 -21:08:38.7
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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
SExtractor catalog cache: saved Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat to cache
SExtractor catalog cache: saved Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Creating symlink local_wcs_cache/wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits exists and is non-empty
wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits exists and is non-empty
wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits exists and is non-empty
wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits (1st reference image)
verification OK: wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Image size: 937.4'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 15:07:04.132 -18:01:06.94 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-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits (1st new image)
verification OK: wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits
Image size: 937.1'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:06:34.485 -18:00:29.85 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:07:04.132 -18:01:06.94
Second-epoch image center 15:06:34.485 -18:00:29.85
Angular distance between the image centers 0.1179 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits (2nd new image)
verification OK: wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
Image size: 937.0'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:06:37.221 -18:00:59.25 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 15:07:04.132 -18:01:06.94
Second-epoch image center 15:06:37.221 -18:00:59.25
Angular distance between the image centers 0.1067 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 15:06:34.485 -18:00:29.85
Second-epoch second image center 15:06:37.221 -18:00:59.25
Angular distance between the image centers 0.01357 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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits &> /tmp/tmp.e4lwli1T5n
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits &> /tmp/tmp.o6b2wt63jv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits &> /tmp/tmp.FpRRJ2NkZc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits &> /tmp/tmp.XhtT3U2k8p
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
Found non-empty wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
The reference image (wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits) and catalog (wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat) found
'wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat' -> 'wcsmag.cat'
Read 42407 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 218.2429 to 235.1834 deg, Dec -23.2935 to -12.5730 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 218.2429 to 235.1834 deg, Dec -23.2935 to -12.5730 deg
Loaded 6189 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): 4998 out of 5340 total matches.
Matched with Tycho-2 5340 out of 42407 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.687465
a=0.000000 b=1.000000 c=22.687465
From vast_summary.log: estimated ref. image limiting mag.: -7.97
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.72
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.72
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 50 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.3 pix Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
2.3 pix Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
2.9 pix fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits
2.9 pix fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
Limiting magnitude estimates:
14.7 mag. Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
14.7 mag. Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
14.7 mag. fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits
14.7 mag. fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.0 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.e4lwli1T5n (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_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits' -> 'wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS_IMAGE_NAME=wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS-calibrated image found: wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Checking if the catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits alredy exist and is non-empty...
Catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS catalog name: wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1940, passed=42401
Got 42401 stars (including 40414 good ones) from the SExtractor catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
util/solve_plate_with_UCAC5 got 42401 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 42016 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 42016 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 42016 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits -region wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.o6b2wt63jv (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_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits' -> 'wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS_IMAGE_NAME=wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS-calibrated image found: wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Checking if the catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits alredy exist and is non-empty...
Catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS catalog name: wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1927, passed=42823
Got 42823 stars (including 40848 good ones) from the SExtractor catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat
util/solve_plate_with_UCAC5 got 42823 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 42414 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 42413 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 42413 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits -region wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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.FpRRJ2NkZc (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_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.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_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits
WCS_IMAGE_NAME=wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits
WCS-calibrated image found: wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits
Checking if the catalog wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits
WCS catalog name: wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=3605, passed=40116
Got 40116 stars (including 36475 good ones) from the SExtractor catalog wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits.cat
util/solve_plate_with_UCAC5 got 40116 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 39589 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 39588 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 39588 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits -region wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.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.XhtT3U2k8p (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_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.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_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
WCS_IMAGE_NAME=wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
WCS-calibrated image found: wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
Checking if the catalog wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
WCS catalog name: wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=3680, passed=40251
Got 40251 stars (including 36536 good ones) from the SExtractor catalog wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits.cat
util/solve_plate_with_UCAC5 got 40251 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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 39688 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 39686 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 39686 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits -region wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Saving fully-calibrated image wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Saving fully-calibrated image wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.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_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-08-55_20.00sec_-4.90C_LIGHT_0266.fits
Saving fully-calibrated image wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.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_2026-04-16_CI_Lib-03-Q2b1x1_021034_TTUQ2b1x1_30872_eu473GFq/wcs_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267.fits
Preparing the HTML report for the field Lib-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53032.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53033.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53043.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53440.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53496.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53500.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53504.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53510.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53522.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53541.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53564.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53577.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53589.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53593.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53599.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53605.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53622.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53632.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53637.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53641.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53651.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53722.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53741.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out53148.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53218.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53658.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 15s
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 53029_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53029_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:57:08.07 -19:37:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53031_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53031_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:49:41.69 -14:01:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53032_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53032_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:58:34.56 -14:06:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 1.329 6311865663117176832 224.64371734183 -14.11630282469 14.3621 13.6080 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.329#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53033_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53033_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:56:53.98 -17:59:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 0.897 6305434482167430656 224.22469787888 -17.98425209122 13.7440 13.0696 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.897#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53036_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53036_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:49:36.05 -16:13:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53043_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53043_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:40:46.35 -14:14:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 1.626 6311066283803939200 220.19272430029 -14.23511925981 13.9164 13.4180 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.626#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53092_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53092_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:59:21.59 -14:27:58.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53123_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53123_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 15:11:42.81 -21:08:38.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53148_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 53148_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 53218_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 53218_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 53440_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53440_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:38:25.19 -15:04:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 1.822 6286940868386621312 219.60460341208 -15.08134458005 13.8818 13.1470 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.822#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53453_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53453_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:37:29.52 -20:19:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 5.497 6280156984722604544 219.37138067559 -20.32824522318 12.3784 10.5670 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.497#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53468_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53468_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:41:11.36 -17:42:40.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53487_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53487_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 53496_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53496_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:48:16.85 -17:16:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 2.258 6282507396985622528 222.07027079277 -17.27048667070 14.1630 13.5559 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.258#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53499_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53499_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:51:30.26 -13:57:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53500_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53500_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:39:44.96 -13:59:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 1.653 6311088377115741952 219.93686596766 -13.99823845150 14.0662 13.4936 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.653#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53504_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53504_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:43:50.99 -15:11:13.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)
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Considering the candidate 53510_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53510_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:38:21.29 -15:09:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 0.641 6286938153967280256 219.58854465866 -15.15180418493 14.2869 13.6493 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.641#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53514_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53514_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:57:03.23 -16:18:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53517_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53517_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 15:02:24.19 -18:46:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53522_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53522_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:45:31.87 -15:36:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 1.385 6309934783259765376 221.38239249842 -15.60526029440 14.2672 13.7865 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.385#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53529_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53529_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:43:55.00 -17:05:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53541_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53541_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:41:58.79 -16:49:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 3.239 6285682717847042560 220.49445716643 -16.81793341187 13.3706 12.0918 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53546_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53546_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:42:14.87 -18:23:56.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53550_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53550_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:45:40.23 -15:18:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53552_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53552_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:49:26.75 -21:34:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53564_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53564_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:43:59.80 -21:27:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 0.792 6279056785900167680 220.99896850593 -21.45209201550 14.5172 13.9112 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.792#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53577_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53577_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:39:20.41 -19:13:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 1.882 6281801682319016192 219.83452330951 -19.23170525865 14.2561 13.6228 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.882#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53581_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53581_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:50:30.81 -19:14:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53589_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53589_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:49:56.73 -21:16:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 2.453 6280332837863872384 222.48575529483 -21.27580495190 13.6396 12.5305 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.453#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53593_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53593_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:55:56.40 -15:26:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 1.129 6307114982611124352 223.98467970707 -15.44594405096 14.1943 13.4614 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.129#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53599_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53599_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:41:15.72 -19:51:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 1.574 6281686641618737152 220.31524139905 -19.85835882839 14.2753 13.7337 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.574#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53601_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53601_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:45:15.13 -20:15:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53605_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53605_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:46:05.23 -17:27:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 1.568 6285480270268473984 221.52146322106 -17.45247505150 14.0871 13.2821 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.568#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53609_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53609_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:47:38.13 -16:22:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53622_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53622_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:38:29.68 -20:14:40.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.33, MAG_FAINT_SEARCH_LIMIT=15.31)
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Considering the candidate 53627_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 53627_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 53631_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53631_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:41:26.83 -21:29:50.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53632_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53632_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:42:04.79 -19:38:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 1.796 6281714954043148160 220.51951557091 -19.63753159155 14.3651 13.7406 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.796#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53637_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53637_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:41:40.49 -19:51:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 1.399 6281500209974606080 220.41905429065 -19.86484297130 14.2695 13.6485 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.399#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53641_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53641_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:50:07.94 -17:30:25.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 0.714 6282443586655428608 222.53304502475 -17.50736151623 14.2566 13.5569 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.714#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53651_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53651_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:48:45.32 -18:23:40.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 1.298 6282092537504497536 222.18883070332 -18.39499939411 14.7101 14.1648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.298#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53658_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
Preparing report for the candidate 53658_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
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Considering the candidate 53675_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53675_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:50:04.95 -21:41:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53676_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53676_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:52:18.56 -20:53:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53722_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53722_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 15:07:09.32 -17:09:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 0.864 6305815359867305344 226.78908366848 -17.15921328514 14.2829 13.6068 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53741_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 53741_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 15:05:53.38 -21:43:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.25, MAG_FAINT_SEARCH_LIMIT=15.23)GAIADR2_OUTPUT=# 1.240 6231729682272595328 226.47276604039 -21.72077365961 14.2226 13.6012 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.240#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 10485_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 10485_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks
**** FOUND 14:42:46.41 -20:12:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23565_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267
The candidate 23565_fd_Lib-03-Q2b1x1_2026-04-16_02-09-51_20.00sec_-4.90C_LIGHT_0267 did not pass the final checks