This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 04 23.4088 2461153.9088 11.65 14:17:15.70 -12:56:54.4
333.11101 44.83558 galactic Vir Second-epoch detections are separated by 1.0" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.154 Bertha 1 -1 1 11.6 -0 0
Forced photometry on wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits at 14:17:15.70 -12:56:54.4: 15.29 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits at 14:17:15.70 -12:56:54.4: 15.30 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 23.4088* 14 17 15.70 -12 56 54.4 11.7 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461153.9088,11.65,0.05,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 20260423.4088 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.4088 2461153.9088 11.93 14:39:37.46 -13:58:25.0
338.85726 41.23055 galactic Lib Second-epoch detections are separated by 0.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.79 Eurynome 1 -0 1 11.8 -0 -0
Forced photometry on wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits at 14:39:37.46 -13:58:25.0: 15.40 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits at 14:39:37.46 -13:58:25.0: 15.41 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461153.9088,11.93,0.05,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 20260423.4088 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.4088 2461153.9088 12.68 14:33:38.64 -11:56:03.4
338.66610 43.73289 galactic Lib Second-epoch detections are separated by 0.7" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.599 Luisa 0 0 0 12.8 0 -0
Forced photometry on wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits at 14:33:38.64 -11:56:03.4: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits at 14:33:38.64 -11:56:03.4: 15.56 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461153.9088,12.68,0.05,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 20260423.4088 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.4088 2461153.9088 14.33 14:48:06.48 -06:09:54.0
347.52726 46.35856 galactic Lib Second-epoch detections are separated by 1.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1107 Lictoria 1 -2 2 14.4 -0 0
Forced photometry on wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits at 14:48:06.48 -06:09:54.0: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits at 14:48:06.48 -06:09:54.0: 15.56 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461153.9088,14.33,0.05,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 20260423.4088 14.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.90985984 27.02.2026 09:50:01.890 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
First image: 2461098.90985984 27.02.2026 09:50:01.890 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Last image: 2461153.90904213 23.04.2026 09:48:51.240 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.16
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5951
Objects passed selection criteria: 5937
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 4610.5
Average stars matched: 4128.75 (89.551 %)
Memory usage VmPeak: 111432 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 23 05:00:45 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.90985984 27.02.2026 09:50:01.890 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
First image: 2461098.90985984 27.02.2026 09:50:01.890 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Last image: 2461153.90904213 23.04.2026 09:48:51.240 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 123
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.87
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 12 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): 36261
Objects passed selection criteria: 36176
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 29362.8
Average stars matched: 25662.2 (87.3973 %)
Memory usage VmPeak: 134952 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 23 05:02:27 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
SExtractor catalog cache: saved Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat to cache
SExtractor catalog cache: saved Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461153.90848319
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits exists and is non-empty
Saving wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits to local_wcs_cache/
'wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits' -> 'local_wcs_cache/wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits'
wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits exists and is non-empty
Saving wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits to local_wcs_cache/
'wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits' -> 'local_wcs_cache/wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits'
wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits exists and is non-empty
Saving wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits to local_wcs_cache/
'wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits' -> 'local_wcs_cache/wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits'
wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits exists and is non-empty
Saving wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits to local_wcs_cache/
'wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits' -> 'local_wcs_cache/wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits (1st reference image)
verification OK: wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Image size: 937.3'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 14:34:25.896 -10:01:24.58 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits (1st new image)
verification OK: wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
Image size: 937.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 14:34:25.572 -10:02:33.00 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:34:25.896 -10:01:24.58
Second-epoch image center 14:34:25.572 -10:02:33.00
Angular distance between the image centers 0.0191 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits (2nd new image)
verification OK: wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
Image size: 937.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 14:34:27.558 -10:03:02.95 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 14:34:25.896 -10:01:24.58
Second-epoch image center 14:34:27.558 -10:03:02.95
Angular distance between the image centers 0.0282 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 14:34:25.572 -10:02:33.00
Second-epoch second image center 14:34:27.558 -10:03:02.95
Angular distance between the image centers 0.01165 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits &> /tmp/tmp.hUgQZ4LBs3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits &> /tmp/tmp.ojsjCySa8l
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits &> /tmp/tmp.iDNaBrr3tK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits &> /tmp/tmp.IPALjJGeoP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits and wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits and wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
Found non-empty wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits and wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
The reference image (wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits) and catalog (wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat) found
'wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat' -> 'wcsmag.cat'
Read 5992 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 210.5294 to 226.6314 deg, Dec -15.2867 to -4.6831 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 210.5294 to 226.6314 deg, Dec -15.2867 to -4.6831 deg
Loaded 4504 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3597 out of 3683 total matches.
Matched with Tycho-2 3683 out of 5992 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.914760
a=0.000000 b=1.000000 c=22.914760
From vast_summary.log: estimated ref. image limiting mag.: -8.16
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.75
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.75
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5992 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 210.5294 to 226.6314 deg, Dec -15.2867 to -4.6831 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 210.5294 to 226.6314 deg, Dec -15.2867 to -4.6831 deg
Loaded 4504 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3597 out of 3683 total matches.
Matched with Tycho-2 3683 out of 5992 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits -> calib.txt_param_ref_wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits (aperture=6.5)
Read 5931 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 210.4988 to 226.6313 deg, Dec -15.3096 to -4.6831 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 210.4988 to 226.6313 deg, Dec -15.3096 to -4.6831 deg
Loaded 4520 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): 3577 out of 3680 total matches.
Matched with Tycho-2 3680 out of 5931 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits -> calib.txt_param_ref_wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits (aperture=6.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.5 pix Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
2.4 pix Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
2.5 pix fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
2.5 pix fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
2.5 pix wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
2.4 pix wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
Limiting magnitude estimates:
14.8 mag. Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
14.8 mag. Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
14.8 mag. fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
14.8 mag. fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 11.8 (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.hUgQZ4LBs3 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits 567.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits' -> 'wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
WCS_IMAGE_NAME=wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
WCS-calibrated image found: wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Checking if the catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits alredy exist and is non-empty...
Catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
WCS catalog name: wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=377, passed=5992
Got 5992 stars (including 5611 good ones) from the SExtractor catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
util/solve_plate_with_UCAC5 got 5992 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 5896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 5898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 5899 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 971 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits -region wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ojsjCySa8l (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits 567.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits' -> 'wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
WCS_IMAGE_NAME=wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
WCS-calibrated image found: wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
Checking if the catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits alredy exist and is non-empty...
Catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
WCS catalog name: wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=404, passed=5931
Got 5931 stars (including 5520 good ones) from the SExtractor catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat
util/solve_plate_with_UCAC5 got 5931 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 5841 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 5841 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 5841 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits -region wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.iDNaBrr3tK (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
WCS_IMAGE_NAME=wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
WCS-calibrated image found: wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
Checking if the catalog wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
WCS catalog name: wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=373, passed=5994
Got 5994 stars (including 5614 good ones) from the SExtractor catalog wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits.cat
util/solve_plate_with_UCAC5 got 5994 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 5916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 5915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 5915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits -region wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.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.IPALjJGeoP (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
WCS_IMAGE_NAME=wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
WCS-calibrated image found: wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
Checking if the catalog wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
WCS catalog name: wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=367, passed=6041
Got 6041 stars (including 5670 good ones) from the SExtractor catalog wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits.cat
util/solve_plate_with_UCAC5 got 6041 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 5967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 5965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 5965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits -region wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits'
Saving fully-calibrated image wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits'
Preparing the HTML report for the field Lib-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out21067.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
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 20457_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 20457_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:46:16.75 -11:05:48.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20716_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 20716_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:42:00.62 -05:49:57.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21067_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
Preparing report for the candidate 21067_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01128_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 01128_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:28:45.18 -13:28:56.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Lib-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
14:17:15.70 -12:56:54.4
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
SExtractor catalog cache: saved Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat to cache
SExtractor catalog cache: saved Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Creating symlink local_wcs_cache/wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits exists and is non-empty
wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits exists and is non-empty
wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits exists and is non-empty
wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits (1st reference image)
verification OK: wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Image size: 937.3'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 14:34:25.896 -10:01:24.58 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits (1st new image)
verification OK: wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
Image size: 937.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 14:34:25.572 -10:02:33.00 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:34:25.896 -10:01:24.58
Second-epoch image center 14:34:25.572 -10:02:33.00
Angular distance between the image centers 0.0191 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits (2nd new image)
verification OK: wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
Image size: 937.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 14:34:27.558 -10:03:02.95 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 14:34:25.896 -10:01:24.58
Second-epoch image center 14:34:27.558 -10:03:02.95
Angular distance between the image centers 0.0282 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 14:34:25.572 -10:02:33.00
Second-epoch second image center 14:34:27.558 -10:03:02.95
Angular distance between the image centers 0.01165 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits &> /tmp/tmp.XbAi1Nw7Nr
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits &> /tmp/tmp.dhH3sfNG8d
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits &> /tmp/tmp.F45g338LjL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits &> /tmp/tmp.WKTHvpFGWx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits and wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits and wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
Found non-empty wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits and wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
The reference image (wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits) and catalog (wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat) found
'wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat' -> 'wcsmag.cat'
Read 33758 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 210.4848 to 226.6346 deg, Dec -15.2985 to -4.6504 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 210.4848 to 226.6346 deg, Dec -15.2985 to -4.6504 deg
Loaded 4537 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3660 out of 3887 total matches.
Matched with Tycho-2 3887 out of 33758 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.758633
a=0.000000 b=1.000000 c=22.758633
From vast_summary.log: estimated ref. image limiting mag.: -7.87
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.89
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.89
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 33758 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 210.4848 to 226.6346 deg, Dec -15.2985 to -4.6504 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 210.4848 to 226.6346 deg, Dec -15.2985 to -4.6504 deg
Loaded 4537 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3660 out of 3887 total matches.
Matched with Tycho-2 3887 out of 33758 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits -> calib.txt_param_ref_wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits (aperture=5.0)
Read 34777 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 210.4845 to 226.6312 deg, Dec -15.3096 to -4.6646 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 210.4845 to 226.6312 deg, Dec -15.3096 to -4.6646 deg
Loaded 4535 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): 3627 out of 3888 total matches.
Matched with Tycho-2 3888 out of 34777 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits -> calib.txt_param_ref_wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 52 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
2.3 pix Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
2.2 pix fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
2.3 pix fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
2.4 pix wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
2.3 pix wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
Limiting magnitude estimates:
14.9 mag. Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
14.9 mag. Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
15.0 mag. fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
15.0 mag. fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.XbAi1Nw7Nr (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits 567.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits' -> 'wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
WCS_IMAGE_NAME=wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
WCS-calibrated image found: wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Checking if the catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits alredy exist and is non-empty...
Catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
WCS catalog name: wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1364, passed=33749
Got 33749 stars (including 32349 good ones) from the SExtractor catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
util/solve_plate_with_UCAC5 got 33749 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 33427 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 33427 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 33427 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits -region wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.dhH3sfNG8d (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits 567.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits' -> 'wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
WCS_IMAGE_NAME=wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
WCS-calibrated image found: wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
Checking if the catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits alredy exist and is non-empty...
Catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
WCS catalog name: wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1488, passed=34765
Got 34765 stars (including 33244 good ones) from the SExtractor catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat
util/solve_plate_with_UCAC5 got 34765 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 34386 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 34386 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 34386 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits -region wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.F45g338LjL (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
WCS_IMAGE_NAME=wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
WCS-calibrated image found: wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
Checking if the catalog wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
WCS catalog name: wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1801, passed=36553
Got 36553 stars (including 34704 good ones) from the SExtractor catalog wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits.cat
util/solve_plate_with_UCAC5 got 36553 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 36106 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 36106 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 36105 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits -region wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.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.WKTHvpFGWx (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
WCS_IMAGE_NAME=wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
WCS-calibrated image found: wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
Checking if the catalog wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
WCS catalog name: wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1775, passed=36219
Got 36219 stars (including 34394 good ones) from the SExtractor catalog wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits.cat
util/solve_plate_with_UCAC5 got 36219 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 35716 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 35717 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 35716 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits -region wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-02_20.00sec_-5.00C_LIGHT_0274.fits
Saving fully-calibrated image wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Lib-01-Q2b1x1_045642_TTUQ2b1x1_423301_vngCz5PV/wcs_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275.fits
Preparing the HTML report for the field Lib-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52773.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52780.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52783.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58694.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58878.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out59408.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out59425.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out59636.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out53898.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54750.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58718.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: 2s
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Considering the candidate 52769_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 52769_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:26:33.07 -07:00:21.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52773_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 52773_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:35:17.80 -12:49:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 1.024 6323458226525498240 218.82445459894 -12.82884366039 14.3470 13.6646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.024#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52777_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 52777_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:43:56.53 -09:58:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52779_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 52779_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:45:26.35 -13:11:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52780_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 52780_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:36:34.18 -12:29:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 2.792 6323575908629531648 219.14163044414 -12.48530589225 14.4864 13.8635 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.792#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52781_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 52781_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:28:50.38 -13:42:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52782_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 52782_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:45:19.36 -12:24:56.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52783_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 52783_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:49:54.24 -13:53:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 0.717 6311287143906456320 222.47618364694 -13.88821674727 13.6520 13.1252 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.717#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52786_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 52786_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:42:44.69 -08:44:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52789_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 52789_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:51:32.73 -13:49:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53063_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 53063_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:46:16.76 -11:05:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53681_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 53681_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:17:15.70 -12:56:54.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53898_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
Preparing report for the candidate 53898_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
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Considering the candidate 54674_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 54674_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:32:21.98 -14:10:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54750_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
Preparing report for the candidate 54750_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
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Considering the candidate 54881_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 54881_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:51:32.69 -13:57:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56777_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 56777_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:18:29.35 -09:25:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58078_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 58078_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:46:00.29 -13:52:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58209_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 58209_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:52:33.14 -11:36:59.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58240_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 58240_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:50:07.42 -12:40:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58275_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 58275_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:51:35.28 -14:00:11.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58454_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 58454_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:18:01.16 -07:39:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58485_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 58485_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:52:21.49 -14:01:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58553_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 58553_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:31:12.10 -10:20:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58673_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 58673_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:45:16.35 -13:18:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58694_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 58694_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:51:32.13 -13:51:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 0.761 6311372669591287168 222.88406817955 -13.85051358093 14.2155 13.5841 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.761#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 58703_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 58703_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:47:41.03 -14:03:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58718_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
Preparing report for the candidate 58718_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
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Considering the candidate 58735_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 58735_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:52:08.46 -10:20:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58859_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 58859_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:17:11.23 -07:45:28.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58878_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 58878_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:49:28.70 -13:49:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 0.497 6311291511889013760 222.36944699425 -13.82707162698 14.2513 13.7171 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.497#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 58881_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 58881_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:48:14.88 -08:36:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58886_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 58886_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:50:41.44 -14:03:48.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58919_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 58919_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:50:18.55 -13:04:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59041_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 59041_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:49:00.20 -13:53:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59068_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 59068_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:29:40.51 -05:57:09.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59155_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 59155_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:48:04.49 -13:25:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59266_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 59266_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:51:30.17 -13:57:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59269_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 59269_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:49:50.97 -13:58:53.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59279_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 59279_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:47:48.72 -06:57:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59325_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 59325_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:43:57.35 -13:54:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59406_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 59406_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:46:58.36 -11:45:29.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59408_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 59408_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:41:05.65 -13:38:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 0.782 6323204235043769984 220.27373659958 -13.64156030552 14.3867 13.8891 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.782#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 59425_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 59425_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:51:45.56 -13:35:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 1.200 6311386207327972736 222.94007180243 -13.59712834473 14.2474 13.6477 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.200#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 59438_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 59438_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:52:06.66 -13:49:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59461_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 59461_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:42:15.97 -14:10:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59542_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 59542_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:42:56.04 -13:42:38.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59604_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 59604_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:23:44.17 -14:05:54.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59636_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 59636_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:33:13.92 -13:37:41.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 0.481 6299338686623634176 218.30810878977 -13.62814064566 14.3521 13.8372 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.481#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 59785_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 59785_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:18:14.19 -09:47:15.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 04974_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 04974_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks
**** FOUND 14:28:45.18 -13:28:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25642_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275
The candidate 25642_fd_Lib-01-Q2b1x1_2026-04-23_04-48-51_20.00sec_-4.90C_LIGHT_0275 did not pass the final checks