This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4
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 07 17.3777 2461238.8777 11.10 21:59:13.68 -11:01:19.3
46.11050 -46.51224 galactic Aqr Second-epoch detections are separated by 0.5" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.354 Eleonora -0 -0 0 11.0 -0 -0
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 21:59:13.68 -11:01:19.3: 15.23 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits at 21:59:13.68 -11:01:19.3: 15.33 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461238.8777,11.10,0.05,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 20260717.3777 11.10CV 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 07 17.3777 2461238.8777 11.62 22:28:59.50 -11:48:51.1
50.51730 -53.28084 galactic Aqr Second-epoch detections are separated by 0.2" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.100 Hekate -0 0 0 11.8 0 0
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:28:59.50 -11:48:51.1: 15.20 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits at 22:28:59.50 -11:48:51.1: 15.31 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461238.8777,11.62,0.05,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 20260717.3777 11.62CV 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 07 17.3777 2461238.8777 13.64 22:24:20.99 -09:38:35.3
52.60585 -51.18837 galactic Aqr Second-epoch detections are separated by 1.3" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.736 Harvard -1 -0 1 13.7 0 0
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:24:20.99 -09:38:35.3: 15.41 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits at 22:24:20.99 -09:38:35.3: 15.53 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461238.8777,13.64,0.05,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 20260717.3777 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.3777 2461238.8777 13.97 21:59:19.41 -07:23:33.3
50.63863 -44.73714 galactic Aqr Second-epoch detections are separated by 1.3" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.286 Iclea -1 1 1 14.0 -0 -0
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 21:59:19.41 -07:23:33.3: 15.38 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits at 21:59:19.41 -07:23:33.3: 15.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461238.8777,13.97,0.05,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 20260717.3777 13.97CV 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 07 17.3777 2461238.8777 14.34 22:25:21.84 -09:27:18.9
53.07187 -51.30113 galactic Aqr Second-epoch detections are separated by 0.8" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1082 Pirola -0 -0 0 14.6 -0 -0
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:25:21.84 -09:27:18.9: 15.43 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits at 22:25:21.84 -09:27:18.9: 15.59 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461238.8777,14.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260717.3777 14.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461211.88265034 20.06.2026 09:10:50.989 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
First image: 2461211.88265034 20.06.2026 09:10:50.989 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
Last image: 2461238.87798797 17.07.2026 09:04:08.161 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.96
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: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 4810
Objects passed selection criteria: 4809
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: 4614.5
Average stars matched: 4330.25 (93.8401 %)
Memory usage VmPeak: 115108 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Jul 16 05:04:38 CDT 2026
VaST build number 1.0rc89-156-g3b0d8dc3
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 17 04:11:05 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: 2461211.88265034 20.06.2026 09:10:50.989 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
First image: 2461211.88265034 20.06.2026 09:10:50.989 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
Last image: 2461238.87798797 17.07.2026 09:04:08.161 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 40
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.65
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: 19 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 30870
Objects passed selection criteria: 30781
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: 29773.2
Average stars matched: 27705.8 (93.0558 %)
Memory usage VmPeak: 136896 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Jul 16 05:04:38 CDT 2026
VaST build number 1.0rc89-156-g3b0d8dc3
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 17 04:13:24 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
SExtractor catalog cache: saved Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.cat to cache
SExtractor catalog cache: saved Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.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/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461238.87744612
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_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits exists and is non-empty
Saving wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits to local_wcs_cache/
'wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits' -> 'local_wcs_cache/wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits'
wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits exists and is non-empty
Saving wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits to local_wcs_cache/
'wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits' -> 'local_wcs_cache/wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits'
wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits exists and is non-empty
Saving wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits to local_wcs_cache/
'wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits' -> 'local_wcs_cache/wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits'
wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits exists and is non-empty
Saving wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits to local_wcs_cache/
'wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits' -> 'local_wcs_cache/wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits (1st reference image)
verification OK: wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
Image size: 937.3'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:07.716 -09:59:55.69 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits (1st new image)
verification OK: wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits
Image size: 937.2'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:09.366 -09:59:40.10 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:17:07.716 -09:59:55.69
Second-epoch image center 22:17:09.366 -09:59:40.10
Angular distance between the image centers 0.0080 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits (2nd new image)
verification OK: wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
Image size: 937.2'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:10.964 -09:58:50.70 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:17:07.716 -09:59:55.69
Second-epoch image center 22:17:10.964 -09:58:50.70
Angular distance between the image centers 0.0224 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 22:17:09.366 -09:59:40.10
Second-epoch second image center 22:17:10.964 -09:58:50.70
Angular distance between the image centers 0.01521 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/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits &> /tmp/tmp.mOiMgBMAHp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits &> /tmp/tmp.LJRP3iKdir
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits &> /tmp/tmp.oFCKtlM3qr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits &> /tmp/tmp.3o7j18NPQp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.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_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits and wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.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_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits and wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat
Found non-empty wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits and wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat
The reference image (wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits) and catalog (wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat) found
'wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat' -> 'wcsmag.cat'
Read 5318 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2566 to 342.3670 deg, Dec -15.2671 to -4.6696 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 326.2566 to 342.3670 deg, Dec -15.2671 to -4.6696 deg
Loaded 5068 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): 3783 out of 3855 total matches.
Matched with Tycho-2 3855 out of 5318 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.567300
a=0.000000 b=1.000000 c=22.567300
From vast_summary.log: estimated ref. image limiting mag.: -7.96
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.61
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.61
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5318 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2566 to 342.3670 deg, Dec -15.2671 to -4.6696 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 326.2566 to 342.3670 deg, Dec -15.2671 to -4.6696 deg
Loaded 5068 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): 3783 out of 3855 total matches.
Matched with Tycho-2 3855 out of 5318 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits -> calib.txt_param_ref_wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits (aperture=6.2)
Read 5828 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2518 to 342.4128 deg, Dec -15.2681 to -4.6697 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 326.2518 to 342.4128 deg, Dec -15.2681 to -4.6697 deg
Loaded 5088 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): 3958 out of 4038 total matches.
Matched with Tycho-2 4038 out of 5828 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits -> calib.txt_param_ref_wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
2.3 pix Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
2.2 pix fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits
2.3 pix fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
2.3 pix wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
2.3 pix wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
Limiting magnitude estimates:
14.6 mag. Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
14.7 mag. Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
14.9 mag. fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits
14.9 mag. fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 11.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.mOiMgBMAHp (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits' -> 'wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
WCS-calibrated image found: wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
Checking if the catalog wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
WCS catalog name: wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.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=331, bad_region=1173, passed=5318
Got 5318 stars (including 3871 good ones) from the SExtractor catalog wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat
util/solve_plate_with_UCAC5 got 5318 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 882 matched stars entering correct_measured_positions(), 881 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 882 matched stars entering correct_measured_positions(), 4256 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 882 matched stars entering correct_measured_positions(), 4254 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 882 matched stars entering correct_measured_positions(), 4254 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 882 stars left (next iteration limit 970)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits N_match=882 sigma_overall_arcsec=0.383 sigma_q1_arcsec=0.390 sigma_q2_arcsec=0.356 sigma_q3_arcsec=0.386 sigma_q4_arcsec=0.423 n_q1=315 n_q2=147 n_q3=286 n_q4=134 worst_quadrant_to_overall_ratio=1.105
The image catalog is written to wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits -region wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.LJRP3iKdir (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits' -> 'wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
WCS-calibrated image found: wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
Checking if the catalog wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
WCS catalog name: wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.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=366, bad_region=1318, passed=5828
Got 5828 stars (including 4212 good ones) from the SExtractor catalog wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat
util/solve_plate_with_UCAC5 got 5828 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 879 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 879 matched stars entering correct_measured_positions(), 875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 879 matched stars entering correct_measured_positions(), 4663 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 879 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 879 matched stars entering correct_measured_positions(), 4664 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 879 matched stars entering correct_measured_positions(), 4664 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 879 stars left (next iteration limit 966)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits N_match=879 sigma_overall_arcsec=0.396 sigma_q1_arcsec=0.363 sigma_q2_arcsec=0.335 sigma_q3_arcsec=0.438 sigma_q4_arcsec=0.419 n_q1=310 n_q2=149 n_q3=288 n_q4=132 worst_quadrant_to_overall_ratio=1.106
The image catalog is written to wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits -region wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.oFCKtlM3qr (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_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.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_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits
Checking if the catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits
WCS catalog name: wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.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=399, bad_region=1321, passed=6282
Got 6282 stars (including 4639 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits.wcscat
util/solve_plate_with_UCAC5 got 6282 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 876 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 876 matched stars entering correct_measured_positions(), 875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 876 matched stars entering correct_measured_positions(), 5137 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 876 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 876 matched stars entering correct_measured_positions(), 5137 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 876 matched stars entering correct_measured_positions(), 5137 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 876 stars left (next iteration limit 963)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits N_match=876 sigma_overall_arcsec=0.384 sigma_q1_arcsec=0.333 sigma_q2_arcsec=0.425 sigma_q3_arcsec=0.431 sigma_q4_arcsec=0.347 n_q1=303 n_q2=151 n_q3=289 n_q4=133 worst_quadrant_to_overall_ratio=1.122
The image catalog is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits -region wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.3o7j18NPQp (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_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.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_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
Checking if the catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
WCS catalog name: wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.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=388, bad_region=1318, passed=6249
Got 6249 stars (including 4618 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits.wcscat
util/solve_plate_with_UCAC5 got 6249 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 875 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 875 matched stars entering correct_measured_positions(), 870 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 875 matched stars entering correct_measured_positions(), 5082 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 875 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 875 matched stars entering correct_measured_positions(), 5082 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 875 matched stars entering correct_measured_positions(), 5082 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 875 stars left (next iteration limit 962)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits N_match=875 sigma_overall_arcsec=0.376 sigma_q1_arcsec=0.362 sigma_q2_arcsec=0.389 sigma_q3_arcsec=0.399 sigma_q4_arcsec=0.350 n_q1=312 n_q2=149 n_q3=284 n_q4=130 worst_quadrant_to_overall_ratio=1.062
The image catalog is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits -region wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits sigma_overall=0.383 worst_q_ratio=1.105
ref2=Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits sigma_overall=0.396 worst_q_ratio=1.106
new1=fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits sigma_overall=0.384 worst_q_ratio=1.122
new2=fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits sigma_overall=0.376 worst_q_ratio=1.062
reference average sigma_overall=0.3895 worst_q_ratio=1.1055
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_astrometric_residuals.png (882 matched stars from wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391_astrometric_residuals.png (879 matched stars from wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212_astrometric_residuals.png (876 matched stars from wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213_astrometric_residuals.png (875 matched stars from wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits'
Saving fully-calibrated image wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits'
Preparing the HTML report for the field Aqr-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 21:59:13.68 -11:01:19.3: 15.23 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:28:59.50 -11:48:51.1: 15.20 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits at 21:59:13.68 -11:01:19.3: 15.33 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits at 22:28:59.50 -11:48:51.1: 15.31 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out20475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20477.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
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
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20467_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213
The candidate 20467_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213 did not pass the final checks
**** FOUND 22:01:42.39 -11:59:40.4 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20475_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213
Preparing report for the candidate 20475_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20477_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213
Preparing report for the candidate 20477_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 10s
Prepared the HTML report for the field Aqr-04-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 ####
21:59:13.68 -11:01:19.3
22:28:59.50 -11:48:51.1
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
SExtractor catalog cache: saved Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.cat to cache
SExtractor catalog cache: saved Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
Creating symlink local_wcs_cache/wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits exists and is non-empty
wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits exists and is non-empty
wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits exists and is non-empty
wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits (1st reference image)
verification OK: wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
Image size: 937.3'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:07.716 -09:59:55.69 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits (1st new image)
verification OK: wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits
Image size: 937.2'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:09.366 -09:59:40.10 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:17:07.716 -09:59:55.69
Second-epoch image center 22:17:09.366 -09:59:40.10
Angular distance between the image centers 0.0080 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits (2nd new image)
verification OK: wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
Image size: 937.2'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:10.964 -09:58:50.70 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:17:07.716 -09:59:55.69
Second-epoch image center 22:17:10.964 -09:58:50.70
Angular distance between the image centers 0.0224 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 22:17:09.366 -09:59:40.10
Second-epoch second image center 22:17:10.964 -09:58:50.70
Angular distance between the image centers 0.01521 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/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits &> /tmp/tmp.s1sOZiFE8w
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits &> /tmp/tmp.vuS1ko8AYD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits &> /tmp/tmp.ceVLZmmVaL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits &> /tmp/tmp.34EHVxMDOo
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.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_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits and wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.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_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits and wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat
Found non-empty wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits and wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat
The reference image (wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits) and catalog (wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat) found
'wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat' -> 'wcsmag.cat'
Read 31665 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2518 to 342.4049 deg, Dec -15.2687 to -4.6696 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 326.2518 to 342.4049 deg, Dec -15.2687 to -4.6696 deg
Loaded 5086 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): 4178 out of 4455 total matches.
Matched with Tycho-2 4455 out of 31665 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.419600
a=0.000000 b=1.000000 c=22.419600
From vast_summary.log: estimated ref. image limiting mag.: -7.65
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.77
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.77
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 31665 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2518 to 342.4049 deg, Dec -15.2687 to -4.6696 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 326.2518 to 342.4049 deg, Dec -15.2687 to -4.6696 deg
Loaded 5086 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): 4178 out of 4455 total matches.
Matched with Tycho-2 4455 out of 31665 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits -> calib.txt_param_ref_wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits (aperture=4.8)
Read 35324 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2518 to 342.4128 deg, Dec -15.2713 to -4.6697 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 326.2518 to 342.4128 deg, Dec -15.2713 to -4.6697 deg
Loaded 5092 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): 4138 out of 4459 total matches.
Matched with Tycho-2 4459 out of 35324 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits -> calib.txt_param_ref_wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 18 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
2.1 pix Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
2.1 pix fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits
2.1 pix fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
2.2 pix wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
2.1 pix wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
Limiting magnitude estimates:
14.8 mag. Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
14.9 mag. Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
15.0 mag. fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits
15.0 mag. fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.s1sOZiFE8w (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits' -> 'wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
WCS-calibrated image found: wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
Checking if the catalog wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
WCS catalog name: wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.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=7, blended=1237, bad_region=4560, passed=31658
Got 31658 stars (including 26107 good ones) from the SExtractor catalog wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat
util/solve_plate_with_UCAC5 got 31658 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 874 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 873 matched stars entering correct_measured_positions(), 869 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 873 matched stars entering correct_measured_positions(), 27571 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 874 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 873 matched stars entering correct_measured_positions(), 27571 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 873 matched stars entering correct_measured_positions(), 27571 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 873 stars left (next iteration limit 960)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits N_match=873 sigma_overall_arcsec=0.388 sigma_q1_arcsec=0.352 sigma_q2_arcsec=0.351 sigma_q3_arcsec=0.432 sigma_q4_arcsec=0.445 n_q1=311 n_q2=145 n_q3=285 n_q4=132 worst_quadrant_to_overall_ratio=1.147
The image catalog is written to wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits -region wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.vuS1ko8AYD (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits' -> 'wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
WCS-calibrated image found: wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
Checking if the catalog wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
WCS catalog name: wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.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=1463, bad_region=5597, passed=35314
Got 35314 stars (including 28476 good ones) from the SExtractor catalog wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat
util/solve_plate_with_UCAC5 got 35314 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 869 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 868 matched stars entering correct_measured_positions(), 866 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 868 matched stars entering correct_measured_positions(), 30582 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 869 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 868 matched stars entering correct_measured_positions(), 30583 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 868 matched stars entering correct_measured_positions(), 30583 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 868 stars left (next iteration limit 954)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits N_match=868 sigma_overall_arcsec=0.382 sigma_q1_arcsec=0.343 sigma_q2_arcsec=0.386 sigma_q3_arcsec=0.421 sigma_q4_arcsec=0.403 n_q1=302 n_q2=153 n_q3=280 n_q4=133 worst_quadrant_to_overall_ratio=1.102
The image catalog is written to wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits -region wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ceVLZmmVaL (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_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.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_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits
Checking if the catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits
WCS catalog name: wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.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=20, blended=1556, bad_region=6439, passed=37945
Got 37945 stars (including 30193 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits.wcscat
util/solve_plate_with_UCAC5 got 37945 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 867 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 866 matched stars entering correct_measured_positions(), 862 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 866 matched stars entering correct_measured_positions(), 32323 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 867 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 866 matched stars entering correct_measured_positions(), 32324 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 866 matched stars entering correct_measured_positions(), 32324 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 866 stars left (next iteration limit 952)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits N_match=866 sigma_overall_arcsec=0.393 sigma_q1_arcsec=0.350 sigma_q2_arcsec=0.416 sigma_q3_arcsec=0.442 sigma_q4_arcsec=0.363 n_q1=303 n_q2=152 n_q3=286 n_q4=125 worst_quadrant_to_overall_ratio=1.124
The image catalog is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits -region wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.34EHVxMDOo (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_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.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_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
Checking if the catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
WCS catalog name: wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.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=19, blended=1518, bad_region=6377, passed=37890
Got 37890 stars (including 30212 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits.wcscat
util/solve_plate_with_UCAC5 got 37890 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 870 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 869 matched stars entering correct_measured_positions(), 865 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 869 matched stars entering correct_measured_positions(), 32375 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 870 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 869 matched stars entering correct_measured_positions(), 32375 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 869 matched stars entering correct_measured_positions(), 32375 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 869 stars left (next iteration limit 955)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits N_match=869 sigma_overall_arcsec=0.389 sigma_q1_arcsec=0.382 sigma_q2_arcsec=0.370 sigma_q3_arcsec=0.435 sigma_q4_arcsec=0.326 n_q1=305 n_q2=150 n_q3=289 n_q4=125 worst_quadrant_to_overall_ratio=1.121
The image catalog is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits -region wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
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_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.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_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-03-21_20.00sec_4.90C_LIGHT_0212.fits
Saving fully-calibrated image wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.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_2026-07-17_CI_Aqr-04-Q2b1x1_040523_TTUQ2b1x1_379213_DDE7bpP4/wcs_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213.fits
Preparing the HTML report for the field Aqr-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:35:00.89 -10:08:10.0: 13.57 +/- 0.07 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:17:02.74 -13:05:36.1: 14.02 +/- 0.11 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 21:59:19.41 -07:23:33.3: 15.38 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:24:20.99 -09:38:35.3: 15.41 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:13:24.90 -09:46:07.4: 14.07 +/- 0.10 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:22:29.33 -14:15:09.7: 12.59 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:18:31.41 -06:04:14.8: 13.80 +/- 0.08 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:06:35.81 -06:38:15.6: 13.37 +/- 0.06 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 21:56:49.27 -13:20:36.2: 14.15 +/- 0.15 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits at 22:17:02.74 -13:05:36.1: 14.32 +/- 0.12 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits at 22:35:00.89 -10:08:10.0: 13.60 +/- 0.07 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits at 22:18:31.41 -06:04:14.8: 13.74 +/- 0.07 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits at 22:24:20.99 -09:38:35.3: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits at 22:06:35.81 -06:38:15.6: 13.45 +/- 0.05 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits at 22:13:24.90 -09:46:07.4: 13.99 +/- 0.08 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits at 21:59:19.41 -07:23:33.3: 15.54 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.16 +/- 0.08
Forced photometry filter REJECTED candidate at 22:17:02.74 -13:05:36.1: ref_mag=14.16 +/- 0.08 new_mean_mag=14.3048 delta=-0.15 (need > 0.90)
Forced photometry reference-image weighted average: 13.59 +/- 0.05
Forced photometry reference-image weighted average: 13.77 +/- 0.05
Forced photometry reference-image weighted average: 13.41 +/- 0.04
Forced photometry reference-image weighted average: 14.02 +/- 0.06
Forced photometry filter REJECTED candidate at 22:18:31.41 -06:04:14.8: ref_mag=13.77 +/- 0.05 new_mean_mag=13.9912 delta=-0.22 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:35:00.89 -10:08:10.0: ref_mag=13.59 +/- 0.05 new_mean_mag=13.8387 delta=-0.25 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:06:35.81 -06:38:15.6: ref_mag=13.41 +/- 0.04 new_mean_mag=13.6883 delta=-0.28 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:13:24.90 -09:46:07.4: ref_mag=14.02 +/- 0.06 new_mean_mag=14.1732 delta=-0.15 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits at 22:22:29.33 -14:15:09.7: 12.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.02
Forced photometry filter REJECTED candidate at 22:22:29.33 -14:15:09.7: ref_mag=12.56 +/- 0.02 new_mean_mag=13.0296 delta=-0.47 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 21:53:41.68 -13:17:38.4: 14.32 +/- 0.16 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits at 21:56:49.27 -13:20:36.2: 14.35 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.11
Forced photometry filter REJECTED candidate at 21:56:49.27 -13:20:36.2: ref_mag=14.25 +/- 0.11 new_mean_mag=14.1142 delta=0.13 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits at 21:53:41.68 -13:17:38.4: 14.53 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.42 +/- 0.12
Forced photometry filter REJECTED candidate at 21:53:41.68 -13:17:38.4: ref_mag=14.42 +/- 0.12 new_mean_mag=14.2757 delta=0.14 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:25:21.84 -09:27:18.9: 15.43 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:05:34.72 -09:54:46.7: 14.78 +/- 0.21 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 21:52:00.92 -06:54:45.3: 14.63 +/- 0.20 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 21:50:00.65 -11:37:25.5: 14.43 +/- 0.20 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:34:58.97 -07:16:04.9: 14.90 +/- 0.26 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits at 22:25:21.84 -09:27:18.9: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits at 21:52:00.92 -06:54:45.3: 14.73 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.68 +/- 0.14
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits at 22:34:58.97 -07:16:04.9: 14.89 +/- 0.21 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits at 21:50:00.65 -11:37:25.5: 14.34 +/- 0.17 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits at 22:05:34.72 -09:54:46.7: 14.28 +/- 0.12 detection
Forced photometry filter REJECTED candidate at 21:52:00.92 -06:54:45.3: ref_mag=14.68 +/- 0.14 new_mean_mag=14.3247 delta=0.35 (need > 0.90)
Forced photometry reference-image weighted average: 14.89 +/- 0.16
Forced photometry reference-image weighted average: 14.41 +/- 0.11
Forced photometry reference-image weighted average: 14.38 +/- 0.13
Forced photometry filter REJECTED candidate at 22:05:34.72 -09:54:46.7: ref_mag=14.41 +/- 0.11 new_mean_mag=14.2644 delta=0.14 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:34:58.97 -07:16:04.9: ref_mag=14.89 +/- 0.16 new_mean_mag=14.3957 delta=0.50 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:50:00.65 -11:37:25.5: ref_mag=14.38 +/- 0.13 new_mean_mag=14.2049 delta=0.18 (need > 0.90)
Adding exclusion_list_local.txt__out54071.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54105.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54207.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
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 53980_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213
The candidate 53980_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 53986_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213
The candidate 53986_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 53988_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213
The candidate 53988_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 53991_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213
The candidate 53991_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 53993_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213
The candidate 53993_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 54001_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213
The candidate 54001_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213 did not pass the final checks
**** FOUND 21:59:13.68 -11:01:19.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 54006_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213
The candidate 54006_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213 did not pass the final checks
**** FOUND 22:28:59.48 -11:48:51.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 54071_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213
Preparing report for the candidate 54071_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213
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Considering the candidate 54096_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213
The candidate 54096_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 54105_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213
Preparing report for the candidate 54105_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213
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Considering the candidate 54106_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213
The candidate 54106_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 54121_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213
The candidate 54121_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213 did not pass the final checks
**** FOUND 22:06:33.90 -13:51:16.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 54139_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213
The candidate 54139_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 54157_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213
The candidate 54157_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 54160_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213
The candidate 54160_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 54185_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213
The candidate 54185_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213 did not pass the final checks
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Considering the candidate 54207_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213
Preparing report for the candidate 54207_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213
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Considering the candidate 54208_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213
The candidate 54208_fd_Aqr-04-Q2b1x1_2026-07-17_04-04-08_20.00sec_5.00C_LIGHT_0213 did not pass the final checks