This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 10 19.3401 2461332.8401 13.14 02:56:03.73 +23:32:39.8
156.55549 -31.06876 galactic Ari Second-epoch detections are separated by 0.5" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.188 Menippe -0 0 0 13.2 0 0
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:56:03.73 +23:32:39.8: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:56:03.73 +23:32:39.8: 16.20 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 19.3401* 02 56 03.73 +23 32 39.8 13.1 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461332.8401,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261019.3401 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 19.3401 2461332.8401 13.44 03:01:07.65 +21:29:24.7
159.03008 -32.13949 galactic Ari Second-epoch detections are separated by 0.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.514 Armida -0 0 0 13.6 0 0
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:01:07.65 +21:29:24.7: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:01:07.65 +21:29:24.7: 16.22 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 19.3401* 03 01 07.65 +21 29 24.7 13.4 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461332.8401,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261019.3401 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 19.3401 2461332.8401 14.22 03:07:47.02 +21:31:05.2
160.50175 -31.22873 galactic Ari Second-epoch detections are separated by 1.3" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.640 Brambilla -0 0 0 14.4 0 0
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:07:47.02 +21:31:05.2: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:07:47.02 +21:31:05.2: 16.11 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 19.3401* 03 07 47.02 +21 31 05.2 14.2 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461332.8401,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261019.3401 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 19.3401 2461332.8401 14.79 03:00:47.72 +25:32:57.1
156.35039 -28.80028 galactic Ari Second-epoch detections are separated by 0.8" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1077 Campanula 0 0 0 14.7 0 0
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:00:47.72 +25:32:57.1: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:00:47.72 +25:32:57.1: 16.14 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 19.3401* 03 00 47.72 +25 32 57.1 14.8 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461332.8401,14.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261019.3401 14.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 19.3401 2461332.8401 14.78 02:28:59.90 +21:04:56.6
151.50033 -36.31922 galactic Ari Second-epoch detections are separated by 0.8" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.935 Clivia -0 -1 1 14.7 0 0
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:59.90 +21:04:56.6: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:59.90 +21:04:56.6: 16.27 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 19.3401* 02 28 59.90 +21 04 56.6 14.8 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461332.8401,14.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261019.3401 14.78CV 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: 2461049.66774773 09.01.2026 04:01:23.404 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
First image: 2461049.66774773 09.01.2026 04:01:23.404 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Last image: 2461332.84035862 19.10.2026 08:09:56.985 /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.28
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 7347
Objects passed selection criteria: 7345
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 7122
Average stars matched: 6888.75 (96.7249 %)
Memory usage VmPeak: 233944 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Oct 19 03:18:21 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: 2461049.66774773 09.01.2026 04:01:23.404 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
First image: 2461049.66774773 09.01.2026 04:01:23.404 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Last image: 2461332.84035862 19.10.2026 08:09:56.985 /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 66
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -6.98
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 15 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 43575
Objects passed selection criteria: 43483
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 42174.2
Average stars matched: 40729 (96.5731 %)
Memory usage VmPeak: 266568 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Oct 19 03:19:11 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
SExtractor catalog cache: saved Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.cat to cache
SExtractor catalog cache: saved Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.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/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
Checking WCS cache directory local_wcs_cache
Checking 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: 2461332.83986150
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_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits exists and is non-empty
wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits exists and is non-empty
wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits exists and is non-empty
wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits (1st reference image)
verification OK: wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 02:46:09.152 +22:00:01.48 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits (1st new image)
verification OK: wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits
Image size: 937.1'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 02:46:10.015 +21:59:49.60 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 02:46:09.152 +22:00:01.48
Second-epoch image center 02:46:10.015 +21:59:49.60
Angular distance between the image centers 0.0047 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits (2nd new image)
verification OK: wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
Image size: 937.1'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 02:46:07.649 +21:59:30.64 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 02:46:09.152 +22:00:01.48
Second-epoch image center 02:46:07.649 +21:59:30.64
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 02:46:10.015 +21:59:49.60
Second-epoch second image center 02:46:07.649 +21:59:30.64
Angular distance between the image centers 0.01055 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits &> /tmp/tmp.khYNLa8Xmn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits &> /tmp/tmp.DNsdJTyJSp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits &> /tmp/tmp.AJ5p61xtjw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits &> /tmp/tmp.6yMBbGi5Qh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
Calibrating the magnitude scale
Found non-empty wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.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_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits and wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits and wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat
Found non-empty wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits and wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat
The reference image (wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits) and catalog (wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat) found
'wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat' -> 'wcsmag.cat'
Read 9126 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 32.8260 to 50.3988 deg, Dec +16.4916 to +27.2900 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 32.8260 to 50.3988 deg, Dec 16.4916 to 27.2900 deg
Loaded 5491 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): 4327 out of 4596 total matches.
Matched with Tycho-2 4596 out of 9126 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.948700
a=0.000000 b=1.000000 c=22.948700
From vast_summary.log: estimated ref. image limiting mag.: -7.28
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.67
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.67
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 9126 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 32.8260 to 50.3988 deg, Dec +16.4916 to +27.2900 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 32.8260 to 50.3988 deg, Dec 16.4916 to 27.2900 deg
Loaded 5491 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): 4327 out of 4596 total matches.
Matched with Tycho-2 4596 out of 9126 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Forced-photometry filter: calibrated wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits -> calib.txt_param_ref_wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits (aperture=6.0)
Read 9076 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 32.7970 to 50.3462 deg, Dec +16.4915 to +27.2889 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 32.7970 to 50.3462 deg, Dec 16.4915 to 27.2889 deg
Loaded 5484 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): 4335 out of 4603 total matches.
Matched with Tycho-2 4603 out of 9076 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
Forced-photometry filter: calibrated wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits -> calib.txt_param_ref_wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
2.0 pix Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
2.3 pix fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits
2.3 pix fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
Limiting magnitude estimates:
15.7 mag. Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
15.7 mag. Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
15.6 mag. fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits
15.6 mag. fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
All-image limiting magnitude estimate: 15.6 (SNR ) 12.4 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.khYNLa8Xmn (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits' -> 'wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
WCS_IMAGE_NAME=wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
WCS-calibrated image found: wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Checking if the catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat corresponding to the image wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits alredy exist and is non-empty...
Catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat corresponding to the image wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
WCS catalog name: wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=637, bad_region=2094, passed=9126
Got 9126 stars (including 6525 good ones) from the SExtractor catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat
util/solve_plate_with_UCAC5 got 9126 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4892 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 4886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 7469 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4893 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 7469 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 7469 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4887 stars left (next iteration limit 5374)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits N_match=4887 sigma_overall_arcsec=0.306 sigma_q1_arcsec=0.373 sigma_q2_arcsec=0.300 sigma_q3_arcsec=0.273 sigma_q4_arcsec=0.257 n_q1=1673 n_q2=881 n_q3=1464 n_q4=869 worst_quadrant_to_overall_ratio=1.222
WCS_HEADER_DIAG: file=Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits selection=current_pairs N_selected=4887 N_valid=4887 bias_ra_arcsec=-0.001 bias_dec_arcsec=-0.003 median_sep_arcsec=0.251 p95_sep_arcsec=0.775 n_q1=1673 n_q2=881 n_q3=1464 n_q4=869 occupied_cells_4x4=16/16
The image catalog is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits -region wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.DNsdJTyJSp (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits' -> 'wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
WCS_IMAGE_NAME=wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
WCS-calibrated image found: wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
Checking if the catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat corresponding to the image wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits alredy exist and is non-empty...
Catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat corresponding to the image wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
WCS catalog name: wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=628, bad_region=2087, passed=9076
Got 9076 stars (including 6485 good ones) from the SExtractor catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat
util/solve_plate_with_UCAC5 got 9076 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4895 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4888 matched stars entering correct_measured_positions(), 4888 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4888 matched stars entering correct_measured_positions(), 7417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4896 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4889 matched stars entering correct_measured_positions(), 7417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4889 matched stars entering correct_measured_positions(), 7417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4889 stars left (next iteration limit 5376)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits N_match=4889 sigma_overall_arcsec=0.300 sigma_q1_arcsec=0.365 sigma_q2_arcsec=0.284 sigma_q3_arcsec=0.280 sigma_q4_arcsec=0.256 n_q1=1669 n_q2=883 n_q3=1466 n_q4=871 worst_quadrant_to_overall_ratio=1.216
WCS_HEADER_DIAG: file=Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits selection=current_pairs N_selected=4889 N_valid=4889 bias_ra_arcsec=0.002 bias_dec_arcsec=-0.001 median_sep_arcsec=0.253 p95_sep_arcsec=0.730 n_q1=1669 n_q2=883 n_q3=1466 n_q4=871 occupied_cells_4x4=16/16
The image catalog is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits -region wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.AJ5p61xtjw (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_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.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_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits
WCS_IMAGE_NAME=wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits
WCS-calibrated image found: wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits
Checking if the catalog wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits.wcscat corresponding to the image wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits alredy exist and is non-empty...
Catalog wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits.wcscat corresponding to the image wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits
WCS catalog name: wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=492, bad_region=2052, passed=9385
Got 9385 stars (including 6912 good ones) from the SExtractor catalog wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits.wcscat
util/solve_plate_with_UCAC5 got 9385 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 533 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4894 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 4887 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 7753 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 533 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4896 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4889 matched stars entering correct_measured_positions(), 7753 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4889 matched stars entering correct_measured_positions(), 7753 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4889 stars left (next iteration limit 5375)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4889 robust_rms=7.855 arcsec worst_region_rms=12.830 arcsec outer_annulus_rms=12.830 arcsec
SIP_REFIT: SIP order 3 trial: matched=4889 robust_rms=0.377 arcsec worst_region_rms=0.727 arcsec outer_annulus_rms=0.727 arcsec
SIP_REFIT: SIP order 5 trial: matched=4889 robust_rms=0.297 arcsec worst_region_rms=0.477 arcsec outer_annulus_rms=0.477 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4889 robust_rms_before=0.883 arcsec robust_rms_before_corrected=0.305 arcsec robust_rms_after=0.297 arcsec worst_region_rms_before=0.514 worst_region_rms_after=0.477 outer_annulus_rms_before=1.119 outer_annulus_rms_after=0.477
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.514 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits worst_region_rms_kept=0.514 arcsec robust_rms_kept=0.305 arcsec matched=4889
WCS_QUALITY_DIAG: file=fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits N_match=4889 sigma_overall_arcsec=0.316 sigma_q1_arcsec=0.286 sigma_q2_arcsec=0.323 sigma_q3_arcsec=0.332 sigma_q4_arcsec=0.335 n_q1=1697 n_q2=882 n_q3=1443 n_q4=867 worst_quadrant_to_overall_ratio=1.061
WCS_HEADER_DIAG: file=fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits selection=current_pairs N_selected=4889 N_valid=4889 bias_ra_arcsec=-0.569 bias_dec_arcsec=0.554 median_sep_arcsec=0.853 p95_sep_arcsec=1.643 n_q1=1697 n_q2=882 n_q3=1443 n_q4=867 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits -region wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.6yMBbGi5Qh (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_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.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_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
WCS_IMAGE_NAME=wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
WCS-calibrated image found: wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
Checking if the catalog wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits.wcscat corresponding to the image wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits alredy exist and is non-empty...
Catalog wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits.wcscat corresponding to the image wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
WCS catalog name: wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=505, bad_region=2044, passed=9347
Got 9347 stars (including 6882 good ones) from the SExtractor catalog wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits.wcscat
util/solve_plate_with_UCAC5 got 9347 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 533 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4893 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 4886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 7706 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 533 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4893 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 7706 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 7706 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4886 stars left (next iteration limit 5374)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4886 robust_rms=7.888 arcsec worst_region_rms=12.877 arcsec outer_annulus_rms=12.877 arcsec
SIP_REFIT: SIP order 3 trial: matched=4886 robust_rms=0.401 arcsec worst_region_rms=0.679 arcsec outer_annulus_rms=0.679 arcsec
SIP_REFIT: SIP order 5 trial: matched=4886 robust_rms=0.314 arcsec worst_region_rms=0.473 arcsec outer_annulus_rms=0.473 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4886 robust_rms_before=0.889 arcsec robust_rms_before_corrected=0.317 arcsec robust_rms_after=0.314 arcsec worst_region_rms_before=0.506 worst_region_rms_after=0.473 outer_annulus_rms_before=1.131 outer_annulus_rms_after=0.473
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.506 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits worst_region_rms_kept=0.506 arcsec robust_rms_kept=0.317 arcsec matched=4886
WCS_QUALITY_DIAG: file=fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits N_match=4886 sigma_overall_arcsec=0.337 sigma_q1_arcsec=0.303 sigma_q2_arcsec=0.345 sigma_q3_arcsec=0.362 sigma_q4_arcsec=0.356 n_q1=1702 n_q2=879 n_q3=1439 n_q4=866 worst_quadrant_to_overall_ratio=1.073
WCS_HEADER_DIAG: file=fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits selection=current_pairs N_selected=4886 N_valid=4886 bias_ra_arcsec=-0.571 bias_dec_arcsec=0.551 median_sep_arcsec=0.854 p95_sep_arcsec=1.666 n_q1=1702 n_q2=879 n_q3=1439 n_q4=866 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits -region wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits to local_wcs_cache/
'wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits' -> 'local_wcs_cache/wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits'
Saving the final (post-refit) wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits to local_wcs_cache/
'wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits' -> 'local_wcs_cache/wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits'
Saving the final (post-refit) wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits to local_wcs_cache/
'wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits' -> 'local_wcs_cache/wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits'
Saving the final (post-refit) wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits to local_wcs_cache/
'wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits' -> 'local_wcs_cache/wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits sigma_overall=0.306 worst_q_ratio=1.222
ref2=Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits sigma_overall=0.300 worst_q_ratio=1.216
new1=fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits sigma_overall=0.316 worst_q_ratio=1.061
new2=fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits sigma_overall=0.337 worst_q_ratio=1.073
reference average sigma_overall=0.303 worst_q_ratio=1.219
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131_astrometric_residuals.png (4887 matched stars from wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132_astrometric_residuals.png (4889 matched stars from wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456_astrometric_residuals.png (4889 matched stars from wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457_astrometric_residuals.png (4886 matched stars from wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits'
Saving fully-calibrated image wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits'
Preparing the HTML report for the field Ari-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:11:04.43 +26:03:26.3: 12.40 +/- 0.01 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:11:04.43 +26:03:26.3: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Forced photometry filter REJECTED candidate at 03:11:04.43 +26:03:26.3: ref_mag=12.38 +/- 0.01 new_mean_mag=12.3622 delta=0.01 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 1s
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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20351_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 20351_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
**** FOUND 02:43:16.59 +22:03:34.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20352_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 20352_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Ari-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
SExtractor catalog cache: saved Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.cat to cache
SExtractor catalog cache: saved Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Creating symlink local_wcs_cache/wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
Creating symlink local_wcs_cache/wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits
Creating symlink local_wcs_cache/wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
Checking 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_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits exists and is non-empty
wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits exists and is non-empty
wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits exists and is non-empty
wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits (1st reference image)
verification OK: wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 02:46:09.152 +22:00:01.48 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits (1st new image)
verification OK: wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits
Image size: 937.1'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 02:46:10.015 +21:59:49.60 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 02:46:09.152 +22:00:01.48
Second-epoch image center 02:46:10.015 +21:59:49.60
Angular distance between the image centers 0.0047 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits (2nd new image)
verification OK: wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
Image size: 937.1'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 02:46:07.649 +21:59:30.64 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 02:46:09.152 +22:00:01.48
Second-epoch image center 02:46:07.649 +21:59:30.64
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 02:46:10.015 +21:59:49.60
Second-epoch second image center 02:46:07.649 +21:59:30.64
Angular distance between the image centers 0.01055 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits &> /tmp/tmp.MhxehR5Ztw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits &> /tmp/tmp.BTqRW187xt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits &> /tmp/tmp.mZrh5QlQ0W
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits &> /tmp/tmp.F3Ndb5f6nL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
Calibrating the magnitude scale
Found non-empty wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.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_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits and wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits and wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat
Found non-empty wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits and wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat
The reference image (wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits) and catalog (wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat) found
'wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat' -> 'wcsmag.cat'
Read 54392 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 32.8053 to 50.3988 deg, Dec +16.4759 to +27.2958 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 32.8053 to 50.3988 deg, Dec 16.4759 to 27.2958 deg
Loaded 5502 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): 4040 out of 4639 total matches.
Matched with Tycho-2 4639 out of 54392 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.822300
a=0.000000 b=1.000000 c=22.822300
From vast_summary.log: estimated ref. image limiting mag.: -6.98
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.84
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.84
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 54392 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 32.8053 to 50.3988 deg, Dec +16.4759 to +27.2958 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 32.8053 to 50.3988 deg, Dec 16.4759 to 27.2958 deg
Loaded 5502 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): 4040 out of 4639 total matches.
Matched with Tycho-2 4639 out of 54392 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Forced-photometry filter: calibrated wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits -> calib.txt_param_ref_wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits (aperture=4.6)
Read 54252 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 32.7970 to 50.3828 deg, Dec +16.4755 to +27.2950 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 32.7970 to 50.3828 deg, Dec 16.4755 to 27.2950 deg
Loaded 5501 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): 4037 out of 4639 total matches.
Matched with Tycho-2 4639 out of 54252 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
Forced-photometry filter: calibrated wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits -> calib.txt_param_ref_wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 38 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
1.9 pix Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
2.3 pix fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits
2.3 pix fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
Limiting magnitude estimates:
15.8 mag. Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
15.8 mag. Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
15.7 mag. fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits
15.7 mag. fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
All-image limiting magnitude estimate: 15.7 (SNR ) 14.8 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.MhxehR5Ztw (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits' -> 'wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
WCS_IMAGE_NAME=wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
WCS-calibrated image found: wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Checking if the catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat corresponding to the image wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits alredy exist and is non-empty...
Catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat corresponding to the image wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
WCS catalog name: wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=2743, bad_region=10132, passed=54382
Got 54382 stars (including 41937 good ones) from the SExtractor catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat
util/solve_plate_with_UCAC5 got 54382 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 4886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 46417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 46417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 46417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4886 stars left (next iteration limit 5374)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits N_match=4886 sigma_overall_arcsec=0.293 sigma_q1_arcsec=0.353 sigma_q2_arcsec=0.280 sigma_q3_arcsec=0.269 sigma_q4_arcsec=0.251 n_q1=1667 n_q2=879 n_q3=1477 n_q4=863 worst_quadrant_to_overall_ratio=1.204
WCS_HEADER_DIAG: file=Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits selection=current_pairs N_selected=4886 N_valid=4886 bias_ra_arcsec=-0.003 bias_dec_arcsec=0.002 median_sep_arcsec=0.246 p95_sep_arcsec=0.761 n_q1=1667 n_q2=879 n_q3=1477 n_q4=863 occupied_cells_4x4=16/16
The image catalog is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits -region wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.BTqRW187xt (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits' -> 'wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
WCS_IMAGE_NAME=wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
WCS-calibrated image found: wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
Checking if the catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat corresponding to the image wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits alredy exist and is non-empty...
Catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat corresponding to the image wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
WCS catalog name: wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=2775, bad_region=10166, passed=54247
Got 54247 stars (including 41735 good ones) from the SExtractor catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat
util/solve_plate_with_UCAC5 got 54247 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4886 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4883 matched stars entering correct_measured_positions(), 4883 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4883 matched stars entering correct_measured_positions(), 46261 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4886 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4883 matched stars entering correct_measured_positions(), 46261 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4883 matched stars entering correct_measured_positions(), 46261 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4883 stars left (next iteration limit 5371)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits N_match=4883 sigma_overall_arcsec=0.290 sigma_q1_arcsec=0.351 sigma_q2_arcsec=0.274 sigma_q3_arcsec=0.266 sigma_q4_arcsec=0.240 n_q1=1655 n_q2=882 n_q3=1488 n_q4=858 worst_quadrant_to_overall_ratio=1.209
WCS_HEADER_DIAG: file=Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits selection=current_pairs N_selected=4883 N_valid=4883 bias_ra_arcsec=0.002 bias_dec_arcsec=0.003 median_sep_arcsec=0.240 p95_sep_arcsec=0.704 n_q1=1655 n_q2=882 n_q3=1488 n_q4=858 occupied_cells_4x4=16/16
The image catalog is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits -region wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.mZrh5QlQ0W (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_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.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_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits
WCS_IMAGE_NAME=wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits
WCS-calibrated image found: wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits
Checking if the catalog wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits.wcscat corresponding to the image wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits alredy exist and is non-empty...
Catalog wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits.wcscat corresponding to the image wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits
WCS catalog name: wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=10, blended=2519, bad_region=7888, passed=48427
Got 48427 stars (including 38592 good ones) from the SExtractor catalog wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits.wcscat
util/solve_plate_with_UCAC5 got 48427 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4872 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 4867 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 42421 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4872 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 42421 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 42421 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4867 stars left (next iteration limit 5353)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4867 robust_rms=7.868 arcsec worst_region_rms=12.596 arcsec outer_annulus_rms=12.596 arcsec
SIP_REFIT: SIP order 3 trial: matched=4867 robust_rms=0.385 arcsec worst_region_rms=0.774 arcsec outer_annulus_rms=0.774 arcsec
SIP_REFIT: SIP order 5 trial: matched=4867 robust_rms=0.298 arcsec worst_region_rms=0.470 arcsec outer_annulus_rms=0.470 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4867 robust_rms_before=0.886 arcsec robust_rms_before_corrected=0.306 arcsec robust_rms_after=0.298 arcsec worst_region_rms_before=0.509 worst_region_rms_after=0.470 outer_annulus_rms_before=1.138 outer_annulus_rms_after=0.470
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.509 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits worst_region_rms_kept=0.509 arcsec robust_rms_kept=0.306 arcsec matched=4867
WCS_QUALITY_DIAG: file=fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits N_match=4867 sigma_overall_arcsec=0.319 sigma_q1_arcsec=0.290 sigma_q2_arcsec=0.330 sigma_q3_arcsec=0.328 sigma_q4_arcsec=0.340 n_q1=1690 n_q2=857 n_q3=1462 n_q4=858 worst_quadrant_to_overall_ratio=1.065
WCS_HEADER_DIAG: file=fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits selection=current_pairs N_selected=4867 N_valid=4867 bias_ra_arcsec=-0.568 bias_dec_arcsec=0.555 median_sep_arcsec=0.858 p95_sep_arcsec=1.644 n_q1=1690 n_q2=857 n_q3=1462 n_q4=858 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits -region wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.F3Ndb5f6nL (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_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.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_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
WCS_IMAGE_NAME=wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
WCS-calibrated image found: wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
Checking if the catalog wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits.wcscat corresponding to the image wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits alredy exist and is non-empty...
Catalog wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits.wcscat corresponding to the image wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
WCS catalog name: wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=2572, bad_region=7971, passed=48768
Got 48768 stars (including 38855 good ones) from the SExtractor catalog wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits.wcscat
util/solve_plate_with_UCAC5 got 48768 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4870 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 4866 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 42705 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4870 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 42705 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 42705 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4866 stars left (next iteration limit 5352)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4866 robust_rms=7.863 arcsec worst_region_rms=12.455 arcsec outer_annulus_rms=12.455 arcsec
SIP_REFIT: SIP order 3 trial: matched=4866 robust_rms=0.403 arcsec worst_region_rms=0.716 arcsec outer_annulus_rms=0.716 arcsec
SIP_REFIT: SIP order 5 trial: matched=4866 robust_rms=0.311 arcsec worst_region_rms=0.480 arcsec outer_annulus_rms=0.480 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4866 robust_rms_before=0.890 arcsec robust_rms_before_corrected=0.314 arcsec robust_rms_after=0.311 arcsec worst_region_rms_before=0.501 worst_region_rms_after=0.480 outer_annulus_rms_before=1.136 outer_annulus_rms_after=0.480
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.501 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits worst_region_rms_kept=0.501 arcsec robust_rms_kept=0.314 arcsec matched=4866
WCS_QUALITY_DIAG: file=fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits N_match=4866 sigma_overall_arcsec=0.330 sigma_q1_arcsec=0.300 sigma_q2_arcsec=0.340 sigma_q3_arcsec=0.352 sigma_q4_arcsec=0.351 n_q1=1689 n_q2=863 n_q3=1464 n_q4=850 worst_quadrant_to_overall_ratio=1.065
WCS_HEADER_DIAG: file=fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits selection=current_pairs N_selected=4866 N_valid=4866 bias_ra_arcsec=-0.569 bias_dec_arcsec=0.555 median_sep_arcsec=0.855 p95_sep_arcsec=1.676 n_q1=1689 n_q2=863 n_q3=1464 n_q4=850 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits -region wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.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_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-14_20.00sec_-0.00C_LIGHT_0456.fits
Saving fully-calibrated image wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.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_2026-10-19_CI_Ari-03-Q2b1x1_031607_TTUQ2b1x1_1748483_rxK7jXIJ/wcs_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457.fits
Preparing the HTML report for the field Ari-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:56:03.73 +23:32:39.8: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:06:20.90 +21:10:36.7: 14.54 +/- 0.08 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:40:28.51 +25:36:15.8: 14.40 +/- 0.07 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:03.69 +20:24:28.0: 14.91 +/- 0.11 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:13:28.10 +23:02:12.9: 12.85 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:01:07.65 +21:29:24.7: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:07:47.02 +21:31:05.2: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:41:10.11 +23:37:01.7: 14.36 +/- 0.07 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:57:01.28 +20:56:17.4: 14.60 +/- 0.08 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:53:17.47 +23:29:45.0: 14.39 +/- 0.07 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:03.69 +20:24:28.0: 15.50 +/- 0.19 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:13:28.10 +23:02:12.9: 12.85 +/- 0.02 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:01:07.65 +21:29:24.7: 16.22 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:40:28.51 +25:36:15.8: 14.53 +/- 0.08 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:56:03.73 +23:32:39.8: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:06:20.90 +21:10:36.7: 14.53 +/- 0.08 detection
Forced photometry reference-image weighted average: 15.06 +/- 0.10
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Forced photometry reference-image weighted average: 14.46 +/- 0.05
Forced photometry reference-image weighted average: 14.54 +/- 0.06
Forced photometry filter REJECTED candidate at 02:28:03.69 +20:24:28.0: ref_mag=15.06 +/- 0.10 new_mean_mag=15.1312 delta=-0.07 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:13:28.10 +23:02:12.9: ref_mag=12.85 +/- 0.01 new_mean_mag=12.8073 delta=0.04 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:40:28.51 +25:36:15.8: ref_mag=14.46 +/- 0.05 new_mean_mag=14.4336 delta=0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:06:20.90 +21:10:36.7: ref_mag=14.54 +/- 0.06 new_mean_mag=14.7779 delta=-0.24 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:07:47.02 +21:31:05.2: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:41:10.11 +23:37:01.7: 14.36 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.36 +/- 0.05
Forced photometry filter REJECTED candidate at 02:41:10.11 +23:37:01.7: ref_mag=14.36 +/- 0.05 new_mean_mag=14.4481 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:57:01.28 +20:56:17.4: 14.75 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.66 +/- 0.06
Forced photometry filter REJECTED candidate at 02:57:01.28 +20:56:17.4: ref_mag=14.66 +/- 0.06 new_mean_mag=14.4316 delta=0.23 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:53:17.47 +23:29:45.0: 14.58 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.47 +/- 0.05
Forced photometry filter REJECTED candidate at 02:53:17.47 +23:29:45.0: ref_mag=14.47 +/- 0.05 new_mean_mag=14.4351 delta=0.04 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:54:34.39 +18:51:41.2: 14.38 +/- 0.07 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:36:47.56 +20:42:31.1: 14.63 +/- 0.10 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:00:13.72 +18:01:03.8: 14.37 +/- 0.07 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:00:26.25 +23:22:14.2: 14.73 +/- 0.10 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:36:20.12 +22:55:05.2: 14.59 +/- 0.08 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:28:59.90 +21:04:56.6: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:00:47.72 +25:32:57.1: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:54:34.39 +18:51:41.2: 14.46 +/- 0.07 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:36:47.56 +20:42:31.1: 14.70 +/- 0.10 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:00:26.25 +23:22:14.2: 14.59 +/- 0.09 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:00:13.72 +18:01:03.8: 14.47 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.42 +/- 0.05
Forced photometry reference-image weighted average: 14.67 +/- 0.07
Forced photometry filter REJECTED candidate at 02:54:34.39 +18:51:41.2: ref_mag=14.42 +/- 0.05 new_mean_mag=14.4558 delta=-0.03 (need > 0.90)
Forced photometry reference-image weighted average: 14.65 +/- 0.06
Forced photometry filter REJECTED candidate at 02:36:47.56 +20:42:31.1: ref_mag=14.67 +/- 0.07 new_mean_mag=14.6810 delta=-0.01 (need > 0.90)
Forced photometry reference-image weighted average: 14.41 +/- 0.05
Forced photometry filter REJECTED candidate at 03:00:26.25 +23:22:14.2: ref_mag=14.65 +/- 0.06 new_mean_mag=14.7277 delta=-0.08 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:00:13.72 +18:01:03.8: ref_mag=14.41 +/- 0.05 new_mean_mag=14.5290 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:36:20.12 +22:55:05.2: 14.46 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.52 +/- 0.06
Forced photometry filter REJECTED candidate at 02:36:20.12 +22:55:05.2: ref_mag=14.52 +/- 0.06 new_mean_mag=14.7729 delta=-0.25 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:28:59.90 +21:04:56.6: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:00:47.72 +25:32:57.1: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:58:34.67 +18:08:05.2: 15.50 +/- 0.20 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:56:24.05 +24:43:35.6: 15.41 +/- 0.18 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:07:02.12 +26:10:27.0: 15.12 +/- 0.16 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:00:49.11 +18:36:57.0: 15.54 +/- 0.21 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:39:38.22 +21:53:00.0: 15.46 +/- 0.17 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:07:02.12 +26:10:27.0: 15.02 +/- 0.14 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:56:24.05 +24:43:35.6: 15.48 +/- 0.19 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:58:34.67 +18:08:05.2: 15.55 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.07 +/- 0.10
Forced photometry filter REJECTED candidate at 03:07:02.12 +26:10:27.0: ref_mag=15.07 +/- 0.10 new_mean_mag=15.0916 delta=-0.03 (need > 0.90)
Forced photometry reference-image weighted average: 15.44 +/- 0.13
Forced photometry reference-image weighted average: 15.52 +/- 0.15
Forced photometry filter REJECTED candidate at 02:56:24.05 +24:43:35.6: ref_mag=15.44 +/- 0.13 new_mean_mag=15.0210 delta=0.42 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:58:34.67 +18:08:05.2: ref_mag=15.52 +/- 0.15 new_mean_mag=15.0182 delta=0.50 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:00:49.11 +18:36:57.0: 15.69 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.60 +/- 0.16
Forced photometry filter REJECTED candidate at 03:00:49.11 +18:36:57.0: ref_mag=15.60 +/- 0.16 new_mean_mag=15.1526 delta=0.45 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:39:38.22 +21:53:00.0: 15.38 +/- 0.16 detection
Forced photometry reference-image weighted average: 15.41 +/- 0.12
Forced photometry filter REJECTED candidate at 02:39:38.22 +21:53:00.0: ref_mag=15.41 +/- 0.12 new_mean_mag=15.0783 delta=0.34 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:41:50.10 +18:24:33.9: 15.35 +/- 0.16 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:14:04.00 +25:29:23.4: 15.23 +/- 0.17 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:09:35.33 +24:52:07.1: 15.14 +/- 0.15 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:31:31.59 +18:45:34.6: 15.00 +/- 0.13 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:09:34.35 +20:42:29.6: 15.21 +/- 0.17 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:14:04.00 +25:29:23.4: 15.56 +/- 0.24 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:09:35.33 +24:52:07.1: 15.34 +/- 0.19 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:41:50.10 +18:24:33.9: 15.19 +/- 0.14 detection
Forced photometry reference-image weighted average: 15.34 +/- 0.14
Forced photometry reference-image weighted average: 15.22 +/- 0.12
Forced photometry reference-image weighted average: 15.26 +/- 0.10
Forced photometry filter REJECTED candidate at 03:14:04.00 +25:29:23.4: ref_mag=15.34 +/- 0.14 new_mean_mag=15.0651 delta=0.28 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:09:35.33 +24:52:07.1: ref_mag=15.22 +/- 0.12 new_mean_mag=15.1053 delta=0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:41:50.10 +18:24:33.9: ref_mag=15.26 +/- 0.10 new_mean_mag=15.1020 delta=0.16 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:31:31.59 +18:45:34.6: 15.33 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.11 +/- 0.11
Forced photometry filter REJECTED candidate at 02:31:31.59 +18:45:34.6: ref_mag=15.11 +/- 0.11 new_mean_mag=15.0024 delta=0.10 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:09:34.35 +20:42:29.6: 15.10 +/- 0.14 detection
Forced photometry reference-image weighted average: 15.14 +/- 0.11
Forced photometry filter REJECTED candidate at 03:09:34.35 +20:42:29.6: ref_mag=15.14 +/- 0.11 new_mean_mag=15.1441 delta=-0.00 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:47:38.55 +17:50:34.3: 16.09 +/- 0.32 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:50:15.57 +26:01:16.0: 16.07 +/- 0.31 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:51:49.70 +25:19:15.8: 15.12 +/- 0.13 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:51:49.70 +25:19:15.8: 15.21 +/- 0.14 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:50:15.57 +26:01:16.0: 15.71 +/- 0.23 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:47:38.55 +17:50:34.3: 15.51 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.16 +/- 0.09
Forced photometry filter REJECTED candidate at 02:51:49.70 +25:19:15.8: ref_mag=15.16 +/- 0.09 new_mean_mag=15.0655 delta=0.09 (need > 0.90)
Forced photometry reference-image weighted average: 15.84 +/- 0.18
Forced photometry reference-image weighted average: 15.66 +/- 0.17
Forced photometry filter REJECTED candidate at 02:50:15.57 +26:01:16.0: ref_mag=15.84 +/- 0.18 new_mean_mag=15.0433 delta=0.79 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:47:38.55 +17:50:34.3: ref_mag=15.66 +/- 0.17 new_mean_mag=15.2298 delta=0.43 (need > 0.90)
Adding exclusion_list_local.txt__out67723.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67768.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67932.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68130.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68162.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 67560_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 67560_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
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Considering the candidate 67583_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 67583_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
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Considering the candidate 67585_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 67585_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
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Considering the candidate 67597_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 67597_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
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Considering the candidate 67723_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
Preparing report for the candidate 67723_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
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Considering the candidate 67733_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 67733_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
**** FOUND 02:48:52.15 +25:12:16.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 67742_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 67742_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
**** FOUND 02:33:53.45 +24:49:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67743_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 67743_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
**** FOUND 03:05:34.14 +25:15:31.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 67768_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
Preparing report for the candidate 67768_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
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Considering the candidate 67785_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 67785_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
**** FOUND 02:34:54.52 +22:25:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67932_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
Preparing report for the candidate 67932_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
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Considering the candidate 67992_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 67992_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
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Considering the candidate 67995_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 67995_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
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Considering the candidate 68009_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 68009_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
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Considering the candidate 68013_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 68013_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
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Considering the candidate 68021_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 68021_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
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Considering the candidate 68058_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 68058_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
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Considering the candidate 68090_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 68090_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
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Considering the candidate 68128_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 68128_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
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Considering the candidate 68130_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
Preparing report for the candidate 68130_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
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Considering the candidate 68162_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
Preparing report for the candidate 68162_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
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Considering the candidate 68166_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 68166_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
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Considering the candidate 68191_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 68191_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
**** FOUND 03:04:51.08 +24:20:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 68196_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 68196_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
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Considering the candidate 68211_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 68211_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
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Considering the candidate 68229_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 68229_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
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Considering the candidate 68230_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 68230_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
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Considering the candidate 68234_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 68234_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
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Considering the candidate 68238_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 68238_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
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Considering the candidate 68245_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 68245_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
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Considering the candidate 68251_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 68251_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
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Considering the candidate 68259_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 68259_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
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Considering the candidate 68274_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 68274_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
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Considering the candidate 68279_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 68279_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
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Considering the candidate 68300_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 68300_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
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Considering the candidate 07437_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 07437_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
Rejecting candidate due to large distance (37.7") between the two second-epoch detections
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Considering the candidate 32355_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 32355_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
Rejecting candidate due to large distance (37.3") between the two second-epoch detections
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Considering the candidate 48068_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457
The candidate 48068_fd_Ari-03-Q2b1x1_2026-10-19_03-09-56_20.00sec_-0.00C_LIGHT_0457 did not pass the final checks
