This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.1785* 09 54 59.50 -32 15 26.1 11.5 U Ant 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5462940328816486144,2461136.6785,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5462940328816486144 20260406.1785 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.1785* 09 53 24.05 -32 01 36.2 11.6 U Ant 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5463148304014992256,2461136.6785,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5463148304014992256 20260406.1785 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.1785* 10 40 05.72 -34 25 52.3 9.4 U Ant 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J104006-3425.9,2461136.6785,9.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J104006-3425.9 20260406.1785 9.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.1785* 10 18 29.05 -29 03 06.5 13.1 U Ant 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.6785,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.1785 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.1785* 09 58 26.84 -35 41 11.1 12.2 U Ant 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J095827-3541.2,2461136.6785,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J095827-3541.2 20260406.1785 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.1785* 10 26 00.03 -38 47 52.1 10.9 U Ant 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J102600-3847.9,2461136.6785,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J102600-3847.9 20260406.1785 10.93CV 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
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 06.1785* 10 18 00.22 -32 54 08.6 11.8 U Ant 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
BE Ant,2461136.6785,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
BE Ant 20260406.1785 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.1785* 10 03 49.68 -38 35 36.0 12.6 U Ant 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J100349.60-383536.8,2461136.6785,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J100349.60-383536.8 20260406.1785 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.1785* 10 07 34.93 -30 44 38.3 11.2 U Ant 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J100735-3044.6,2461136.6785,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J100735-3044.6 20260406.1785 11.19CV 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: 2461061.87334150 21.01.2026 08:57:26.706 /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
First image: 2461061.87334150 21.01.2026 08:57:26.706 /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
Last image: 2461136.67991623 06.04.2026 04:18:54.762 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 22
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.33
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: 6 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): 9282
Objects passed selection criteria: 9274
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 8652
Average stars matched: 8253.5 (95.3941 %)
Memory usage VmPeak: 115104 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 5 23:20:53 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: 2461061.87334150 21.01.2026 08:57:26.706 /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
First image: 2461061.87334150 21.01.2026 08:57:26.706 /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
Last image: 2461136.67991623 06.04.2026 04:18:54.762 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 56
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.06
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: 34 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): 63757
Objects passed selection criteria: 63646
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 55810.5
Average stars matched: 53597.8 (96.0352 %)
Memory usage VmPeak: 163076 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 5 23:22:45 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
SExtractor catalog cache: saved Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits.cat to cache
SExtractor catalog cache: saved Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.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/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.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: 2461136.67713142
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_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits exists and is non-empty
Saving wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits to local_wcs_cache/
'wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits' -> 'local_wcs_cache/wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits'
wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits exists and is non-empty
Saving wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits to local_wcs_cache/
'wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits' -> 'local_wcs_cache/wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits'
wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits exists and is non-empty
Saving wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits to local_wcs_cache/
'wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits' -> 'local_wcs_cache/wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits'
wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits exists and is non-empty
Saving wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits to local_wcs_cache/
'wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits' -> 'local_wcs_cache/wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:26:01.730 -34:00:05.44
Second-epoch image center 10:26:06.129 -34:00:19.01
Angular distance between the image centers 0.0157 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:26:01.730 -34:00:05.44
Second-epoch image center 10:26:03.085 -34:00:38.55
Angular distance between the image centers 0.0103 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 10:26:06.129 -34:00:19.01
Second-epoch second image center 10:26:03.085 -34:00:38.55
Angular distance between the image centers 0.01183 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/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits &> /tmp/tmp.iHqOnDUq26
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits &> /tmp/tmp.8TbeXjAyz8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits &> /tmp/tmp.Ay6c4DPmKv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits &> /tmp/tmp.apdsRz6WCH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
Calibrating the magnitude scale
Found non-empty wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.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_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits and wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.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_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits and wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits.cat
Found non-empty wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits and wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits.cat
The reference image (wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits) and catalog (wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits.cat) found
'wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits.cat' -> 'wcsmag.cat'
Read 8859 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 146.3085 to 166.3941 deg, Dec -39.3228 to -28.2857 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 146.3085 to 166.3941 deg, Dec -39.3228 to -28.2857 deg
Loaded 13375 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): 7317 out of 7534 total matches.
Matched with Tycho-2 7534 out of 8859 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.734701
a=0.000000 b=1.000000 c=22.734701
From vast_summary.log: estimated ref. image limiting mag.: -8.33
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.40
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 18 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
2.1 pix Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits
4.9 pix fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits
2.8 pix fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
Limiting magnitude estimates:
14.4 mag. Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
14.4 mag. Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits
13.7 mag. fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits
14.3 mag. fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 11.3 (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.iHqOnDUq26 (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_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits' -> 'wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
WCS_IMAGE_NAME=wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
WCS-calibrated image found: wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
Checking if the catalog wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits.cat corresponding to the image wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits alredy exist and is non-empty...
Catalog wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits.cat corresponding to the image wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
WCS catalog name: wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=616, passed=8859
Got 8859 stars (including 8230 good ones) from the SExtractor catalog wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits.cat
util/solve_plate_with_UCAC5 got 8859 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 8705 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 253 to 310 (Dec -39.3 to -28.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 8705 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
WARNING: Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 8705 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits -region wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.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.8TbeXjAyz8 (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_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits' -> 'wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits
WCS_IMAGE_NAME=wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits
WCS-calibrated image found: wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits
Checking if the catalog wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits.cat corresponding to the image wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits alredy exist and is non-empty...
Catalog wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits.cat corresponding to the image wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits
WCS catalog name: wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=653, passed=8886
Got 8886 stars (including 8224 good ones) from the SExtractor catalog wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits.cat
util/solve_plate_with_UCAC5 got 8886 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 8777 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
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 253 to 310 (Dec -39.3 to -28.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 8777 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
WARNING: Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 8788 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 976 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits -region wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.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.Ay6c4DPmKv (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_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.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_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits
WCS_IMAGE_NAME=wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits
WCS-calibrated image found: wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits
Checking if the catalog wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits.cat corresponding to the image wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits alredy exist and is non-empty...
Catalog wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits.cat corresponding to the image wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits
WCS catalog name: wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=339, passed=7699
Got 7699 stars (including 7359 good ones) from the SExtractor catalog wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits.cat
util/solve_plate_with_UCAC5 got 7699 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.5'
Seting catalog search parameters based on the expected field of view 940.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013063 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010450 (37.6 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 252 to 311 (Dec -39.5 to -28.0)
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...
WARNING: Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 7608 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
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 252 to 311 (Dec -39.5 to -28.0)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 7611 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
WARNING: Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 7611 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits -region wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.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.apdsRz6WCH (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_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.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_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
WCS_IMAGE_NAME=wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
WCS-calibrated image found: wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
Checking if the catalog wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits.cat corresponding to the image wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits alredy exist and is non-empty...
Catalog wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits.cat corresponding to the image wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
WCS catalog name: wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=562, passed=9384
Got 9384 stars (including 8820 good ones) from the SExtractor catalog wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits.cat
util/solve_plate_with_UCAC5 got 9384 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010453 (37.6 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 252 to 311 (Dec -39.5 to -28.0)
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...
WARNING: Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 9245 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 252 to 311 (Dec -39.5 to -28.0)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 9246 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
WARNING: Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 9246 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
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_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits -region wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.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_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits'
Saving fully-calibrated image wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits'
Saving fully-calibrated image wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits'
Saving fully-calibrated image wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits'
Preparing the HTML report for the field Ant-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20613.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20626.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20635.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20638.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20645.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20664.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20665.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20667.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20668.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20672.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20675.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20676.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20677.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out20669.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out04377.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20662.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20673.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 20609_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 20609_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:21:32.72 -34:39:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20613_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 20613_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:07:34.93 -30:44:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 0.822 5460508582754357504 151.89551858428 -30.74374476632 10.7259 9.5898 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.822#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20626_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 20626_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 09:59:26.05 -31:52:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.20, MAG_FAINT_SEARCH_LIMIT=12.18)GAIADR2_OUTPUT=# 0.854 5463011041156522624 149.85835922026 -31.88143137375 10.9265 9.6485 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.854#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20635_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 20635_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:05:25.40 -38:11:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.33, MAG_FAINT_SEARCH_LIMIT=12.31)GAIADR2_OUTPUT=# 0.936 5421470632864005120 151.35561777607 -38.19858609790 10.4150 9.0150 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.936#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20638_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 20638_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:21:24.10 -33:50:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.39, MAG_FAINT_SEARCH_LIMIT=12.37)GAIADR2_OUTPUT=# 1.584 5446807881895689600 155.35061882822 -33.84714894952 10.5265 9.2280 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.584#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20645_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 20645_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:00:59.52 -34:58:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.41, MAG_FAINT_SEARCH_LIMIT=12.39)GAIADR2_OUTPUT=# 1.169 5434662229779565824 150.24767085724 -34.97845799517 10.7242 9.4535 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.169#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20662_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 20662_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20664_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 20664_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:06:19.02 -35:57:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)GAIADR2_OUTPUT=# 1.048 5434332582450212736 151.57891540796 -35.96128225000 10.7297 9.4416 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.048#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20665_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 20665_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:25:33.83 -32:30:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)GAIADR2_OUTPUT=# 0.531 5448475325635999744 156.39079581138 -32.50102673722 11.4534 11.1049 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.531#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20667_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 20667_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:09:55.90 -34:02:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 0.467 5458614712633313792 152.48286735006 -34.04895645206 11.2557 10.5451 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.467#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20668_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 20668_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 09:58:55.31 -30:00:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)GAIADR2_OUTPUT=# 0.471 5463792897002666752 149.73041032087 -30.00123711351 11.3451 10.3131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20669_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 20669_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 09:53:23.33 -29:36:26.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.60, MAG_FAINT_SEARCH_LIMIT=12.58)
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Considering the candidate 20672_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 20672_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:13:07.30 -30:09:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.56, MAG_FAINT_SEARCH_LIMIT=12.54)GAIADR2_OUTPUT=# 1.184 5461878986558678144 153.28003933294 -30.15970899385 11.5310 11.0968 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.184#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20673_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 20673_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20675_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 20675_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:06:08.03 -30:45:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.59, MAG_FAINT_SEARCH_LIMIT=12.57)GAIADR2_OUTPUT=# 0.703 5460552460139500672 151.53323413827 -30.75460651184 11.4616 10.7127 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.703#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20676_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 20676_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 09:49:45.33 -32:32:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)GAIADR2_OUTPUT=# 0.995 5439100511543778688 147.43856611998 -32.53651828965 11.4204 10.6651 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.995#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20677_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 20677_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:09:58.29 -31:55:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)GAIADR2_OUTPUT=# 0.581 5460197253462716800 152.49290505980 -31.92011851044 11.3297 10.5507 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.581#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04377_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 04377_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 19s
Prepared the HTML report for the field Ant-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
10:40:05.72 -34:25:52.3
09:54:59.50 -32:15:26.1
09:53:24.05 -32:01:36.2
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
SExtractor catalog cache: saved Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits.cat to cache
SExtractor catalog cache: saved Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
Creating symlink local_wcs_cache/wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits
Creating symlink local_wcs_cache/wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits
Creating symlink local_wcs_cache/wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.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_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits exists and is non-empty
wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits exists and is non-empty
wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits exists and is non-empty
wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:26:01.730 -34:00:05.44
Second-epoch image center 10:26:06.129 -34:00:19.01
Angular distance between the image centers 0.0157 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:26:01.730 -34:00:05.44
Second-epoch image center 10:26:03.085 -34:00:38.55
Angular distance between the image centers 0.0103 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 10:26:06.129 -34:00:19.01
Second-epoch second image center 10:26:03.085 -34:00:38.55
Angular distance between the image centers 0.01183 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/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits &> /tmp/tmp.hSxsWj6fWU
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits &> /tmp/tmp.OvcwifrT6e
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits &> /tmp/tmp.ymStaEO7cq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits &> /tmp/tmp.jeMrV75B6l
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
Calibrating the magnitude scale
Found non-empty wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.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_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits and wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.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_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits and wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits.cat
Found non-empty wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits and wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits.cat
The reference image (wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits) and catalog (wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits.cat) found
'wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits.cat' -> 'wcsmag.cat'
Read 65964 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 146.2913 to 166.3941 deg, Dec -39.3236 to -28.2647 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 146.2913 to 166.3941 deg, Dec -39.3236 to -28.2647 deg
Loaded 13412 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): 10050 out of 10983 total matches.
Matched with Tycho-2 10983 out of 65964 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.561401
a=0.000000 b=1.000000 c=22.561401
From vast_summary.log: estimated ref. image limiting mag.: -8.06
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.50
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.50
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 39 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
2.0 pix Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits
4.3 pix fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits
2.5 pix fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
Limiting magnitude estimates:
14.5 mag. Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
14.5 mag. Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits
13.9 mag. fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits
14.4 mag. fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 13.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.hSxsWj6fWU (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_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits' -> 'wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
WCS_IMAGE_NAME=wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
WCS-calibrated image found: wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
Checking if the catalog wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits.cat corresponding to the image wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits alredy exist and is non-empty...
Catalog wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits.cat corresponding to the image wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
WCS catalog name: wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=3141, passed=65960
Got 65960 stars (including 62689 good ones) from the SExtractor catalog wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits.cat
util/solve_plate_with_UCAC5 got 65960 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 65297 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 253 to 310 (Dec -39.3 to -28.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 65298 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
WARNING: Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 65298 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits -region wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.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.OvcwifrT6e (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_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits' -> 'wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits
WCS_IMAGE_NAME=wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits
WCS-calibrated image found: wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits
Checking if the catalog wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits.cat corresponding to the image wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits alredy exist and is non-empty...
Catalog wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits.cat corresponding to the image wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits
WCS catalog name: wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=3134, passed=66197
Got 66197 stars (including 62941 good ones) from the SExtractor catalog wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits.cat
util/solve_plate_with_UCAC5 got 66197 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.3)
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...
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 65752 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 253 to 310 (Dec -39.3 to -28.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 65751 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 65751 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
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_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits -region wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.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.ymStaEO7cq (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_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.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_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits
WCS_IMAGE_NAME=wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits
WCS-calibrated image found: wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits
Checking if the catalog wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits.cat corresponding to the image wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits alredy exist and is non-empty...
Catalog wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits.cat corresponding to the image wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits
WCS catalog name: wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=2620, passed=36122
Got 36122 stars (including 33481 good ones) from the SExtractor catalog wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits.cat
util/solve_plate_with_UCAC5 got 36122 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.5'
Seting catalog search parameters based on the expected field of view 940.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013063 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010450 (37.6 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 252 to 312 (Dec -39.5 to -28.0)
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...
WARNING: Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 35595 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
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 252 to 312 (Dec -39.5 to -28.0)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 35593 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
WARNING: Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 35593 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits -region wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.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.jeMrV75B6l (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_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.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_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
WCS_IMAGE_NAME=wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
WCS-calibrated image found: wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
Checking if the catalog wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits.cat corresponding to the image wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits alredy exist and is non-empty...
Catalog wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits.cat corresponding to the image wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
WCS catalog name: wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=20, blended=2668, passed=56702
Got 56702 stars (including 53975 good ones) from the SExtractor catalog wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits.cat
util/solve_plate_with_UCAC5 got 56702 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010453 (37.6 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 252 to 312 (Dec -39.5 to -28.0)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 55979 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 252 to 312 (Dec -39.5 to -28.0)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 55978 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
WARNING: Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 55978 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits -region wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.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_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.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_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/wcs_Ant-02-Q1b1x1_2026-01-21_02-57-26_20.00sec_-15.00C_LIGHT_0424.fits
Saving fully-calibrated image wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.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_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/wcs_Ant-02-Q1b1x1_2026-01-21_02-58-10_20.00sec_-15.00C_LIGHT_0425.fits
Saving fully-calibrated image wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.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_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-14-54_20.00sec_-5.00C_LIGHTs_0066.fits
Saving fully-calibrated image wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.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_2026-04-05_CI_Ant-02-Q1b1x1_231945_TTUQ1b1x1_19194_YqUvHGmw/wcs_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067.fits
Preparing the HTML report for the field Ant-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out20764.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out81575.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out81589.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out81601.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out81621.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out81635.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out81639.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out81651.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out81654.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82181.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82193.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82213.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82235.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82245.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82246.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82252.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82280.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82286.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out81643.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out02941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02998.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21274.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46898.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55777.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82073.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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: 4s
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Considering the candidate 81575_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 81575_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 09:59:03.12 -30:19:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 1.879 5463737268586303232 149.76293951624 -30.32042512687 13.4773 13.0031 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.879#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 81589_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 81589_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:08:22.81 -32:30:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 2.859 5460061463778099456 152.09441758110 -32.50603932319 13.3786 12.9383 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.859#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 81598_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 81598_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:56:45.30 -30:14:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81601_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 81601_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:10:57.86 -35:27:35.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)
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Considering the candidate 81613_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 81613_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 11:01:44.39 -37:46:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81617_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 81617_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:55:44.03 -38:09:52.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81621_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 81621_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 09:48:57.74 -34:24:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 2.812 5438277797670058240 147.23984520192 -34.40331636628 12.1008 11.3779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.812#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 81625_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 81625_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:58:48.20 -37:10:57.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81634_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 81634_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:50:50.47 -38:47:11.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81635_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 81635_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 09:54:07.35 -36:32:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 1.850 5434103639213874176 148.53037790846 -36.53333143759 12.2191 11.7220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 81639_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 81639_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 09:59:04.85 -34:31:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 3.867 5435449377026185728 149.77149008438 -34.52266523612 12.7363 12.0434 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 81643_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 81643_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:52:53.62 -32:55:41.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)
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Considering the candidate 81646_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 81646_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:59:39.20 -38:41:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81649_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 81649_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 11:01:40.66 -39:05:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81651_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 81651_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:04:23.34 -38:30:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 5.794 5421459191075358720 151.09785228802 -38.50890568764 11.8942 11.2567 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 81654_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 81654_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:03:22.01 -37:32:26.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.399 5422075948374438528 150.84170967696 -37.54072197676 11.9440 11.2542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.399#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 81906_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 81906_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:37:24.22 -35:03:54.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82073_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 82073_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 82181_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 82181_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:43:17.21 -30:45:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 0.924 5454326686003605632 160.82180018346 -30.76510535008 13.9488 13.4380 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.924#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82193_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 82193_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 11:02:49.18 -30:14:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 0.598 5452160785535211776 165.70495120508 -30.24664219562 13.5280 12.9582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.598#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82213_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 82213_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:46:33.90 -29:58:29.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)
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Considering the candidate 82235_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 82235_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:45:30.02 -30:17:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 0.857 5454739209022157184 161.37534017047 -30.28389206773 13.9379 13.2849 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.857#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82245_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 82245_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 11:02:13.13 -32:45:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 2.720 5450121157106260224 165.55459198303 -32.75708405798 13.8804 13.3622 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.720#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82246_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 82246_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:45:01.94 -29:52:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.377 5454769857908655616 161.25829492517 -29.87127563442 14.0540 13.0189 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.377#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82252_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 82252_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:54:01.89 -32:52:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.251 5450277871872663808 163.50717581614 -32.87531313265 13.8633 13.1782 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.251#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82265_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 82265_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:26:43.61 -29:13:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 3.340 5461651082711455232 156.68064756159 -29.22057816389 14.1786 13.7077 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.340#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82280_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 82280_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:35:57.82 -29:40:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 1.000 5455420940591837952 158.99063276936 -29.67687217287 14.1666 13.6190 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.000#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82286_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 82286_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:49:01.51 -30:03:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 3.010 5454643757668723968 162.25538443239 -30.05546265238 14.0323 13.5763 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82298_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 82298_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:37:11.10 -29:26:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 1.298 5455446263719047168 159.29603710493 -29.44853148328 14.0540 13.5747 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.298#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31815_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 31815_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:40:05.71 -34:25:52.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 30261_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 30261_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 10:21:32.72 -34:39:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20764_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 20764_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 09:49:59.77 -35:34:09.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)
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Considering the candidate 21274_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 21274_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 02998_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
Preparing report for the candidate 02998_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
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Considering the candidate 65901_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 65901_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
**** FOUND 09:56:15.54 -31:14:36.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14775_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067
The candidate 14775_fd_Ant-02-Q1b1x1_2026-04-05_23-18-54_20.00sec_-5.00C_LIGHTs_0067 did not pass the final checks
