This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 10 11.1709 2461324.6709 11.79 22:04:20.80 -14:35:24.0
42.17491 -49.21841 galactic Aqr Second-epoch detections are separated by 0.1" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.5 Astraea -0 -0 0 11.9 0 0
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:04:20.80 -14:35:24.0: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:04:20.80 -14:35:24.0: 15.52 +/- 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,2461324.6709,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261011.1709 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.1709 2461324.6709 12.82 22:17:14.97 -11:41:17.9
48.40527 -50.71441 galactic Aqr Second-epoch detections are separated by 0.6" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.117 Lomia -0 -0 1 13.0 0 0
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:17:14.97 -11:41:17.9: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:17:14.97 -11:41:17.9: 15.91 +/- 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,2461324.6709,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261011.1709 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.1709 2461324.6709 13.43 21:53:09.62 -11:04:52.8
45.03884 -45.22257 galactic Cap Second-epoch detections are separated by 0.1" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.78 Diana -1 0 1 13.4 -0 -0
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:53:09.62 -11:04:52.8: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:53:09.62 -11:04:52.8: 15.73 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.1709* 21 53 09.62 -11 04 52.8 13.4 U Cap 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461324.6709,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261011.1709 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.1709 2461324.6709 13.80 22:08:06.59 -11:26:31.3
47.08501 -48.63066 galactic Aqr Second-epoch detections are separated by 1.3" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.303 Josephina -1 -0 1 14.1 -0 -0
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:08:06.59 -11:26:31.3: 15.50 +/- 0.27 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:08:06.59 -11:26:31.3: 15.86 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.50 +/- 0.27
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,2461324.6709,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261011.1709 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.1709 2461324.6709 13.89 22:23:32.67 -10:47:18.3
50.87018 -51.61076 galactic Aqr Second-epoch detections are separated by 0.6" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.208 Lacrimosa -1 -0 1 14.0 0 0
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:23:32.67 -10:47:18.3: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:23:32.67 -10:47:18.3: 15.86 +/- 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,2461324.6709,13.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261011.1709 13.89CV 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: 2461242.93279922 21.07.2026 10:23:03.853 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
First image: 2461242.93279922 21.07.2026 10:23:03.853 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Last image: 2461324.67124726 11.10.2026 04:06:25.763 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.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.: -7.38
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 6 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 7172
Objects passed selection criteria: 7170
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 6953.25
Average stars matched: 6734.75 (96.8576 %)
Memory usage VmPeak: 233260 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Oct 9 16:07:04 CDT 2026
VaST build number 1.0rc89-234-g1a8c12b2
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-09)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Oct 10 23:54:09 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: 2461242.93279922 21.07.2026 10:23:03.853 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
First image: 2461242.93279922 21.07.2026 10:23:03.853 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Last image: 2461324.67124726 11.10.2026 04:06:25.763 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 71
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.12
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: 52 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 44321
Objects passed selection criteria: 44201
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 43106.8
Average stars matched: 41522.5 (96.3248 %)
Memory usage VmPeak: 264280 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Oct 9 16:07:04 CDT 2026
VaST build number 1.0rc89-234-g1a8c12b2
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-09)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Oct 10 23:56:44 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
SExtractor catalog cache: saved Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.cat to cache
SExtractor catalog cache: saved Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461324.67049528
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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits exists and is non-empty
wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits exists and is non-empty
wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits exists and is non-empty
wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits (1st reference image)
verification OK: wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:16:59.412 -09:59:39.54 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits (1st new image)
verification OK: wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
Image size: 941.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:17:13.647 -10:00:51.21 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:16:59.412 -09:59:39.54
Second-epoch image center 22:17:13.647 -10:00:51.21
Angular distance between the image centers 0.0617 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits (2nd new image)
verification OK: wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
Image size: 941.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:17:11.677 -10:01:30.17 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:16:59.412 -09:59:39.54
Second-epoch image center 22:17:11.677 -10:01:30.17
Angular distance between the image centers 0.0590 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 22:17:13.647 -10:00:51.21
Second-epoch second image center 22:17:11.677 -10:01:30.17
Angular distance between the image centers 0.01351 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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits &> /tmp/tmp.dPnNMIfuMz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits &> /tmp/tmp.2JItT0iYJa
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits &> /tmp/tmp.jr9mn7237S
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits &> /tmp/tmp.B4kvaZtYxp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits and wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits and wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
Found non-empty wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits and wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
The reference image (wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits) and catalog (wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat) found
'wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat' -> 'wcsmag.cat'
Read 6925 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.8536 to 342.4026 deg, Dec -15.6017 to -4.2140 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 325.8536 to 342.4026 deg, Dec -15.6017 to -4.2140 deg
Loaded 5569 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): 4112 out of 4275 total matches.
Matched with Tycho-2 4275 out of 6925 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.673200
a=0.000000 b=1.000000 c=22.673200
From vast_summary.log: estimated ref. image limiting mag.: -7.38
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.29
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.29
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6925 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.8536 to 342.4026 deg, Dec -15.6017 to -4.2140 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 325.8536 to 342.4026 deg, Dec -15.6017 to -4.2140 deg
Loaded 5569 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): 4112 out of 4275 total matches.
Matched with Tycho-2 4275 out of 6925 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Forced-photometry filter: calibrated wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits -> calib.txt_param_ref_wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits (aperture=5.8)
Read 6918 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.8535 to 342.3813 deg, Dec -15.6029 to -4.2885 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 325.8535 to 342.3813 deg, Dec -15.6029 to -4.2885 deg
Loaded 5525 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): 4139 out of 4302 total matches.
Matched with Tycho-2 4302 out of 6918 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
Forced-photometry filter: calibrated wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits -> calib.txt_param_ref_wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits (aperture=5.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
2.1 pix Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
2.2 pix fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
2.2 pix fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
Limiting magnitude estimates:
15.3 mag. Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
15.3 mag. Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
15.3 mag. fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
15.3 mag. fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.dPnNMIfuMz (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_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits' -> 'wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
WCS-calibrated image found: wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Checking if the catalog wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
WCS catalog name: wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=496, bad_region=0, passed=6925
Got 6925 stars (including 6418 good ones) from the SExtractor catalog wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
util/solve_plate_with_UCAC5 got 6925 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4341 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4318 matched stars entering correct_measured_positions(), 4318 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4318 matched stars entering correct_measured_positions(), 6925 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4341 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4318 matched stars entering correct_measured_positions(), 6925 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4318 matched stars entering correct_measured_positions(), 6925 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4318 stars left (next iteration limit 4749)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits N_match=4318 sigma_overall_arcsec=0.352 sigma_q1_arcsec=0.347 sigma_q2_arcsec=0.393 sigma_q3_arcsec=0.316 sigma_q4_arcsec=0.319 n_q1=1030 n_q2=1223 n_q3=924 n_q4=1141 worst_quadrant_to_overall_ratio=1.115
The image catalog is written to wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits -region wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.2JItT0iYJa (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_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.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-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits' -> 'wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
WCS-calibrated image found: wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
Checking if the catalog wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
WCS catalog name: wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=479, bad_region=0, passed=6918
Got 6918 stars (including 6429 good ones) from the SExtractor catalog wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat
util/solve_plate_with_UCAC5 got 6918 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4340 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4319 matched stars entering correct_measured_positions(), 4319 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4318 matched stars entering correct_measured_positions(), 6918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4338 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4316 matched stars entering correct_measured_positions(), 6918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4316 matched stars entering correct_measured_positions(), 6918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4316 stars left (next iteration limit 4749)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits N_match=4316 sigma_overall_arcsec=0.331 sigma_q1_arcsec=0.333 sigma_q2_arcsec=0.389 sigma_q3_arcsec=0.296 sigma_q4_arcsec=0.300 n_q1=1033 n_q2=1228 n_q3=924 n_q4=1131 worst_quadrant_to_overall_ratio=1.177
The image catalog is written to wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits -region wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.jr9mn7237S (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
Checking if the catalog wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
WCS catalog name: wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=507, bad_region=0, passed=7084
Got 7084 stars (including 6568 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits.wcscat
util/solve_plate_with_UCAC5 got 7084 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4348 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4324 matched stars entering correct_measured_positions(), 4324 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4324 matched stars entering correct_measured_positions(), 7084 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4346 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4322 matched stars entering correct_measured_positions(), 7084 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4322 matched stars entering correct_measured_positions(), 7084 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 4322 stars left (next iteration limit 4756)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4322 robust_rms=14.492 arcsec worst_region_rms=23.697 arcsec outer_annulus_rms=23.697 arcsec
SIP_REFIT: SIP order 3 trial: matched=4322 robust_rms=0.464 arcsec worst_region_rms=0.621 arcsec outer_annulus_rms=0.621 arcsec
SIP_REFIT: SIP order 5 trial: matched=4322 robust_rms=0.265 arcsec worst_region_rms=0.294 arcsec outer_annulus_rms=0.292 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4322 robust_rms_before=0.937 arcsec robust_rms_before_corrected=0.286 arcsec robust_rms_after=0.265 arcsec worst_region_rms_before=0.327 worst_region_rms_after=0.294 outer_annulus_rms_before=0.938 outer_annulus_rms_after=0.292
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.327 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits worst_region_rms_kept=0.327 arcsec robust_rms_kept=0.286 arcsec matched=4322
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits N_match=4322 sigma_overall_arcsec=0.290 sigma_q1_arcsec=0.298 sigma_q2_arcsec=0.341 sigma_q3_arcsec=0.247 sigma_q4_arcsec=0.261 n_q1=1046 n_q2=1208 n_q3=926 n_q4=1142 worst_quadrant_to_overall_ratio=1.176
The image catalog is written to wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits -region wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.B4kvaZtYxp (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
Checking if the catalog wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
WCS catalog name: wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=497, bad_region=0, passed=7105
Got 7105 stars (including 6597 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits.wcscat
util/solve_plate_with_UCAC5 got 7105 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4344 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4321 matched stars entering correct_measured_positions(), 4321 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4321 matched stars entering correct_measured_positions(), 7105 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4343 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4321 matched stars entering correct_measured_positions(), 7105 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4321 matched stars entering correct_measured_positions(), 7105 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 4321 stars left (next iteration limit 4753)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4321 robust_rms=14.502 arcsec worst_region_rms=23.679 arcsec outer_annulus_rms=23.679 arcsec
SIP_REFIT: SIP order 3 trial: matched=4321 robust_rms=0.469 arcsec worst_region_rms=0.616 arcsec outer_annulus_rms=0.616 arcsec
SIP_REFIT: SIP order 5 trial: matched=4321 robust_rms=0.258 arcsec worst_region_rms=0.290 arcsec outer_annulus_rms=0.290 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4321 robust_rms_before=0.933 arcsec robust_rms_before_corrected=0.284 arcsec robust_rms_after=0.258 arcsec worst_region_rms_before=0.328 worst_region_rms_after=0.290 outer_annulus_rms_before=0.936 outer_annulus_rms_after=0.290
verification OK: wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
verification OK: wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
Image size: 941.3'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:17:11.721 -10:01:30.61 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 7105 stars ###
'wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/correct_sextractor_wcs_catalog_usingxy2sky1613308.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.933 -> 0.258 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (cycle 1, search radius 3.0 arcsec, 4321 pairs from the previous matching)
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4145 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 4145 pairs (4321 from the previous matching)
SIP_REFIT: SIP order 2 trial: matched=4145 robust_rms=14.405 arcsec worst_region_rms=23.945 arcsec outer_annulus_rms=23.945 arcsec
SIP_REFIT: SIP order 3 trial: matched=4145 robust_rms=0.467 arcsec worst_region_rms=0.599 arcsec outer_annulus_rms=0.599 arcsec
SIP_REFIT: SIP order 5 trial: matched=4145 robust_rms=0.258 arcsec worst_region_rms=0.291 arcsec outer_annulus_rms=0.291 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4145 robust_rms_before=0.258 arcsec robust_rms_before_corrected=0.258 arcsec robust_rms_after=0.258 arcsec worst_region_rms_before=0.290 worst_region_rms_after=0.291 outer_annulus_rms_before=0.290 outer_annulus_rms_after=0.291
SIP_REFIT: the refit on the re-matched pairs is worse than the solution it would replace (worst-region 0.291 vs 0.290 arcsec) - keeping the current solution
SIP_REFIT: the refit on the re-matched pairs was not applied - keeping the current solution
Accuracy estimation diagnostic: 4145 matched stars entering correct_measured_positions(), 7105 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Accuracy estimation diagnostic: 4145 matched stars entering correct_measured_positions(), 7105 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits N_match=4145 sigma_overall_arcsec=0.274 sigma_q1_arcsec=0.283 sigma_q2_arcsec=0.312 sigma_q3_arcsec=0.264 sigma_q4_arcsec=0.248 n_q1=988 n_q2=1167 n_q3=896 n_q4=1094 worst_quadrant_to_overall_ratio=1.139
The image catalog is written to wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits -region wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits to local_wcs_cache/
'wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits' -> 'local_wcs_cache/wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits'
Saving the final (post-refit) wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits to local_wcs_cache/
'wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits' -> 'local_wcs_cache/wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits'
Saving the final (post-refit) wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits to local_wcs_cache/
'wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits' -> 'local_wcs_cache/wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits'
Saving the final (post-refit) wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits to local_wcs_cache/
'wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits' -> 'local_wcs_cache/wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits sigma_overall=0.352 worst_q_ratio=1.115
ref2=Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits sigma_overall=0.331 worst_q_ratio=1.177
new1=fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits sigma_overall=0.290 worst_q_ratio=1.176
new2=fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits sigma_overall=0.274 worst_q_ratio=1.139
reference average sigma_overall=0.3415 worst_q_ratio=1.146
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859_astrometric_residuals.png (4318 matched stars from wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860_astrometric_residuals.png (4316 matched stars from wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180_astrometric_residuals.png (4322 matched stars from wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.26 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181_astrometric_residuals.png (4145 matched stars from wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.20 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits'
Saving fully-calibrated image wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits'
Preparing the HTML report for the field Aqr-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:22:11.90 -09:21:06.1: 12.00 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:04:20.80 -14:35:24.0: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:04:05.88 -08:06:08.1: 12.08 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:04:20.80 -14:35:24.0: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:22:11.90 -09:21:06.1: 12.00 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:04:05.88 -08:06:08.1: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Forced photometry filter REJECTED candidate at 22:04:05.88 -08:06:08.1: ref_mag=12.07 +/- 0.01 new_mean_mag=12.0604 delta=0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:22:11.90 -09:21:06.1: ref_mag=12.00 +/- 0.01 new_mean_mag=12.0005 delta=0.00 (need > 0.90)
Adding exclusion_list_local.txt__out20421.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
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 20419_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 20419_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
**** FOUND 22:04:39.84 -07:11:34.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20421_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
Preparing report for the candidate 20421_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
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Considering the candidate 20426_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 20426_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 20430_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 20430_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 11s
Prepared the HTML report for the field Aqr-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
22:04:20.80 -14:35:24.0
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
SExtractor catalog cache: saved Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.cat to cache
SExtractor catalog cache: saved Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Creating symlink local_wcs_cache/wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits exists and is non-empty
wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits exists and is non-empty
wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits exists and is non-empty
wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits (1st reference image)
verification OK: wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:16:59.412 -09:59:39.54 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits (1st new image)
verification OK: wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
Image size: 941.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:17:13.647 -10:00:51.21 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:16:59.412 -09:59:39.54
Second-epoch image center 22:17:13.647 -10:00:51.21
Angular distance between the image centers 0.0617 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits (2nd new image)
verification OK: wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
Image size: 941.3'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:17:11.721 -10:01:30.61 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:16:59.412 -09:59:39.54
Second-epoch image center 22:17:11.721 -10:01:30.61
Angular distance between the image centers 0.0592 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 22:17:13.647 -10:00:51.21
Second-epoch second image center 22:17:11.721 -10:01:30.61
Angular distance between the image centers 0.01350 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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits &> /tmp/tmp.fd3xulWvDE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits &> /tmp/tmp.8hcBuUUB2T
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits &> /tmp/tmp.s8W3GS2UJP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits &> /tmp/tmp.RxcKdVe4pJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits and wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits and wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
Found non-empty wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits and wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
The reference image (wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits) and catalog (wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat) found
'wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat' -> 'wcsmag.cat'
Read 44007 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.8306 to 342.4342 deg, Dec -15.6017 to -4.2093 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 325.8306 to 342.4342 deg, Dec -15.6017 to -4.2093 deg
Loaded 5591 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): 4073 out of 4476 total matches.
Matched with Tycho-2 4476 out of 44007 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.570300
a=0.000000 b=1.000000 c=22.570300
From vast_summary.log: estimated ref. image limiting mag.: -7.12
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.45
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.45
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 44007 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.8306 to 342.4342 deg, Dec -15.6017 to -4.2093 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 325.8306 to 342.4342 deg, Dec -15.6017 to -4.2093 deg
Loaded 5591 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): 4073 out of 4476 total matches.
Matched with Tycho-2 4476 out of 44007 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Forced-photometry filter: calibrated wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits -> calib.txt_param_ref_wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits (aperture=4.6)
Read 43933 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.8257 to 342.4191 deg, Dec -15.6029 to -4.2242 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 325.8257 to 342.4191 deg, Dec -15.6029 to -4.2242 deg
Loaded 5583 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): 4085 out of 4489 total matches.
Matched with Tycho-2 4489 out of 43933 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
Forced-photometry filter: calibrated wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits -> calib.txt_param_ref_wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 57 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
2.0 pix Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
2.1 pix fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
2.1 pix fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
Limiting magnitude estimates:
15.5 mag. Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
15.4 mag. Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
15.4 mag. fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
15.4 mag. fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
All-image limiting magnitude estimate: 15.4 (SNR ) 14.5 (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.fd3xulWvDE (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_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits' -> 'wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
WCS-calibrated image found: wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Checking if the catalog wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
WCS catalog name: wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=23, blended=1813, bad_region=20, passed=43984
Got 43984 stars (including 42059 good ones) from the SExtractor catalog wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
util/solve_plate_with_UCAC5 got 43984 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4331 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4313 matched stars entering correct_measured_positions(), 4313 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4313 matched stars entering correct_measured_positions(), 43984 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4332 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4311 matched stars entering correct_measured_positions(), 43984 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4311 matched stars entering correct_measured_positions(), 43984 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4311 stars left (next iteration limit 4744)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits N_match=4311 sigma_overall_arcsec=0.334 sigma_q1_arcsec=0.328 sigma_q2_arcsec=0.385 sigma_q3_arcsec=0.300 sigma_q4_arcsec=0.311 n_q1=1040 n_q2=1219 n_q3=934 n_q4=1118 worst_quadrant_to_overall_ratio=1.152
The image catalog is written to wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits -region wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.8hcBuUUB2T (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_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.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-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits' -> 'wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
WCS-calibrated image found: wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
Checking if the catalog wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
WCS catalog name: wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=21, blended=1714, bad_region=21, passed=43912
Got 43912 stars (including 42099 good ones) from the SExtractor catalog wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat
util/solve_plate_with_UCAC5 got 43912 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4334 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4315 matched stars entering correct_measured_positions(), 4315 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4315 matched stars entering correct_measured_positions(), 43912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4333 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4314 matched stars entering correct_measured_positions(), 43912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4314 matched stars entering correct_measured_positions(), 43912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4314 stars left (next iteration limit 4746)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits N_match=4314 sigma_overall_arcsec=0.315 sigma_q1_arcsec=0.322 sigma_q2_arcsec=0.369 sigma_q3_arcsec=0.276 sigma_q4_arcsec=0.290 n_q1=1055 n_q2=1210 n_q3=924 n_q4=1125 worst_quadrant_to_overall_ratio=1.171
The image catalog is written to wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits -region wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.s8W3GS2UJP (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
Checking if the catalog wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
WCS catalog name: wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1781, bad_region=34, passed=43108
Got 43108 stars (including 41215 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits.wcscat
util/solve_plate_with_UCAC5 got 43108 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4336 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4317 matched stars entering correct_measured_positions(), 4318 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4317 matched stars entering correct_measured_positions(), 43108 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4335 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4315 matched stars entering correct_measured_positions(), 43108 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4315 matched stars entering correct_measured_positions(), 43108 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 4315 stars left (next iteration limit 4748)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4315 robust_rms=14.566 arcsec worst_region_rms=24.006 arcsec outer_annulus_rms=24.006 arcsec
SIP_REFIT: SIP order 3 trial: matched=4315 robust_rms=0.466 arcsec worst_region_rms=0.643 arcsec outer_annulus_rms=0.643 arcsec
SIP_REFIT: SIP order 5 trial: matched=4315 robust_rms=0.261 arcsec worst_region_rms=0.292 arcsec outer_annulus_rms=0.292 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4315 robust_rms_before=0.933 arcsec robust_rms_before_corrected=0.275 arcsec robust_rms_after=0.261 arcsec worst_region_rms_before=0.318 worst_region_rms_after=0.292 outer_annulus_rms_before=0.937 outer_annulus_rms_after=0.292
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.318 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits worst_region_rms_kept=0.318 arcsec robust_rms_kept=0.275 arcsec matched=4315
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits N_match=4315 sigma_overall_arcsec=0.282 sigma_q1_arcsec=0.292 sigma_q2_arcsec=0.337 sigma_q3_arcsec=0.239 sigma_q4_arcsec=0.251 n_q1=1054 n_q2=1210 n_q3=930 n_q4=1121 worst_quadrant_to_overall_ratio=1.198
The image catalog is written to wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits -region wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.RxcKdVe4pJ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
Checking if the catalog wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
WCS catalog name: wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=9, blended=1743, bad_region=37, passed=42820
Got 42820 stars (including 40968 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits.wcscat
util/solve_plate_with_UCAC5 got 42820 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4328 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4309 matched stars entering correct_measured_positions(), 4310 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4308 matched stars entering correct_measured_positions(), 42820 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4328 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4308 matched stars entering correct_measured_positions(), 42820 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 4308 matched stars entering correct_measured_positions(), 42820 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 4308 stars left (next iteration limit 4738)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4308 robust_rms=14.547 arcsec worst_region_rms=23.758 arcsec outer_annulus_rms=23.758 arcsec
SIP_REFIT: SIP order 3 trial: matched=4308 robust_rms=0.470 arcsec worst_region_rms=0.607 arcsec outer_annulus_rms=0.607 arcsec
SIP_REFIT: SIP order 5 trial: matched=4308 robust_rms=0.255 arcsec worst_region_rms=0.292 arcsec outer_annulus_rms=0.292 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4308 robust_rms_before=0.255 arcsec robust_rms_before_corrected=0.269 arcsec robust_rms_after=0.255 arcsec worst_region_rms_before=0.293 worst_region_rms_after=0.292 outer_annulus_rms_before=0.293 outer_annulus_rms_after=0.292
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.293 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits worst_region_rms_kept=0.293 arcsec robust_rms_kept=0.255 arcsec matched=4308
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits N_match=4308 sigma_overall_arcsec=0.269 sigma_q1_arcsec=0.271 sigma_q2_arcsec=0.312 sigma_q3_arcsec=0.235 sigma_q4_arcsec=0.260 n_q1=1045 n_q2=1215 n_q3=930 n_q4=1118 worst_quadrant_to_overall_ratio=1.162
The image catalog is written to wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits -region wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-05-20_20.00sec_0.00C_LIGHTs_0180.fits
Saving fully-calibrated image wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Aqr-04-Q1b1x1_232851_TTUQ1b1x1_598073_Yu5pl3GR/wcs_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181.fits
Preparing the HTML report for the field Aqr-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:17:14.97 -11:41:17.9: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:12:30.04 -04:54:49.1: 11.21 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:44:53.51 -12:39:24.9: 15.08 +/- 0.25 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:37:48.14 -07:16:09.1: 13.68 +/- 0.05 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:08:06.59 -11:26:31.3: 15.50 +/- 0.27 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:53:09.62 -11:04:52.8: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:44:00.62 -13:36:22.2: 14.22 +/- 0.12 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:23:32.67 -10:47:18.3: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:39:38.41 -14:05:45.6: 14.98 +/- 0.23 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:35:10.13 -14:38:13.6: 15.19 +/- 0.26 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:23:32.67 -10:47:18.3: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:44:53.51 -12:39:24.9: 14.71 +/- 0.18 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:39:38.41 -14:05:45.6: 14.74 +/- 0.17 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:53:09.62 -11:04:52.8: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:08:06.59 -11:26:31.3: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:17:14.97 -11:41:17.9: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:12:30.04 -04:54:49.1: 11.23 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:37:48.14 -07:16:09.1: 13.72 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.83 +/- 0.14
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:44:00.62 -13:36:22.2: 14.19 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.83 +/- 0.14
Forced photometry reference-image weighted average: 15.50 +/- 0.27
Forced photometry filter REJECTED candidate at 22:44:53.51 -12:39:24.9: ref_mag=14.83 +/- 0.14 new_mean_mag=14.5454 delta=0.29 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:39:38.41 -14:05:45.6: ref_mag=14.83 +/- 0.14 new_mean_mag=14.4557 delta=0.37 (need > 0.90)
Forced photometry filter KEPT candidate at 22:08:06.59 -11:26:31.3: ref_mag=15.50 +/- 0.27 new_mean_mag=13.8017 delta=1.70 (need > 0.90)
Forced photometry reference-image weighted average: 11.22 +/- 0.00
Forced photometry reference-image weighted average: 13.70 +/- 0.04
Forced photometry reference-image weighted average: 14.21 +/- 0.08
Forced photometry filter REJECTED candidate at 22:12:30.04 -04:54:49.1: ref_mag=11.22 +/- 0.00 new_mean_mag=11.4543 delta=-0.23 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:37:48.14 -07:16:09.1: ref_mag=13.70 +/- 0.04 new_mean_mag=13.9933 delta=-0.30 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:44:00.62 -13:36:22.2: ref_mag=14.21 +/- 0.08 new_mean_mag=14.2145 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:35:10.13 -14:38:13.6: 15.14 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.16 +/- 0.18
Forced photometry filter REJECTED candidate at 22:35:10.13 -14:38:13.6: ref_mag=15.16 +/- 0.18 new_mean_mag=14.5256 delta=0.64 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:41:08.19 -14:32:02.0: 14.63 +/- 0.18 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:25:46.66 -13:29:00.5: 14.87 +/- 0.16 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:16:11.55 -14:21:24.5: 14.53 +/- 0.13 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:14:09.81 -14:34:34.4: 14.81 +/- 0.16 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:49:58.29 -11:36:00.0: 14.42 +/- 0.13 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:54:24.43 -14:06:38.1: 14.76 +/- 0.17 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:16:11.55 -14:21:24.5: 14.78 +/- 0.16 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:41:08.19 -14:32:02.0: 14.53 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.63 +/- 0.10
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:49:58.29 -11:36:00.0: 14.46 +/- 0.14 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:25:46.66 -13:29:00.5: 14.75 +/- 0.14 detection
Forced photometry filter REJECTED candidate at 22:16:11.55 -14:21:24.5: ref_mag=14.63 +/- 0.10 new_mean_mag=14.5687 delta=0.06 (need > 0.90)
Forced photometry reference-image weighted average: 14.58 +/- 0.12
Forced photometry filter REJECTED candidate at 22:41:08.19 -14:32:02.0: ref_mag=14.58 +/- 0.12 new_mean_mag=14.6163 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:14:09.81 -14:34:34.4: 14.92 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.44 +/- 0.10
Forced photometry reference-image weighted average: 14.80 +/- 0.11
Forced photometry filter REJECTED candidate at 21:49:58.29 -11:36:00.0: ref_mag=14.44 +/- 0.10 new_mean_mag=14.4920 delta=-0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:25:46.66 -13:29:00.5: ref_mag=14.80 +/- 0.11 new_mean_mag=14.5504 delta=0.25 (need > 0.90)
Forced photometry reference-image weighted average: 14.86 +/- 0.12
Forced photometry filter REJECTED candidate at 22:14:09.81 -14:34:34.4: ref_mag=14.86 +/- 0.12 new_mean_mag=14.6093 delta=0.25 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:54:24.43 -14:06:38.1: 15.11 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.88 +/- 0.14
Forced photometry filter REJECTED candidate at 21:54:24.43 -14:06:38.1: ref_mag=14.88 +/- 0.14 new_mean_mag=14.6536 delta=0.23 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:36:36.16 -13:42:44.1: 14.85 +/- 0.18 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:55:45.30 -14:14:44.9: 14.74 +/- 0.17 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:48:02.36 -13:19:58.1: 14.70 +/- 0.19 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:32:51.40 -06:35:35.0: 15.16 +/- 0.20 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:45:35.67 -07:46:56.1: 15.03 +/- 0.22 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:51:29.53 -12:33:31.2: 14.89 +/- 0.19 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:55:45.30 -14:14:44.9: 14.64 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.69 +/- 0.11
Forced photometry filter REJECTED candidate at 21:55:45.30 -14:14:44.9: ref_mag=14.69 +/- 0.11 new_mean_mag=14.6192 delta=0.07 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:36:36.16 -13:42:44.1: 14.88 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.87 +/- 0.13
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:32:51.40 -06:35:35.0: 14.82 +/- 0.14 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:48:02.36 -13:19:58.1: 14.78 +/- 0.21 detection
Forced photometry filter REJECTED candidate at 22:36:36.16 -13:42:44.1: ref_mag=14.87 +/- 0.13 new_mean_mag=14.5849 delta=0.28 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:45:35.67 -07:46:56.1: 15.02 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.93 +/- 0.12
Forced photometry reference-image weighted average: 15.02 +/- 0.15
Forced photometry filter REJECTED candidate at 22:32:51.40 -06:35:35.0: ref_mag=14.93 +/- 0.12 new_mean_mag=14.6905 delta=0.24 (need > 0.90)
Forced photometry reference-image weighted average: 14.74 +/- 0.14
Forced photometry filter REJECTED candidate at 22:45:35.67 -07:46:56.1: ref_mag=15.02 +/- 0.15 new_mean_mag=14.6841 delta=0.34 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:48:02.36 -13:19:58.1: ref_mag=14.74 +/- 0.14 new_mean_mag=14.3967 delta=0.34 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:51:29.53 -12:33:31.2: 14.68 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.76 +/- 0.12
Forced photometry filter REJECTED candidate at 21:51:29.53 -12:33:31.2: ref_mag=14.76 +/- 0.12 new_mean_mag=14.6103 delta=0.15 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:52:08.44 -13:46:47.6: 14.98 +/- 0.21 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:31:06.93 -14:16:07.6: 14.73 +/- 0.15 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:48:39.98 -12:10:46.3: 14.91 +/- 0.18 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:04:24.47 -14:09:22.3: 15.10 +/- 0.21 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:55:01.63 -04:53:27.2: 14.82 +/- 0.15 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:52:08.44 -13:46:47.6: 15.05 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.01 +/- 0.15
Forced photometry filter REJECTED candidate at 21:52:08.44 -13:46:47.6: ref_mag=15.01 +/- 0.15 new_mean_mag=14.6065 delta=0.40 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:31:06.93 -14:16:07.6: 15.08 +/- 0.21 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:56:17.36 -13:15:05.3: 14.87 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.85 +/- 0.13
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:48:39.98 -12:10:46.3: 14.91 +/- 0.18 detection
Forced photometry filter REJECTED candidate at 22:31:06.93 -14:16:07.6: ref_mag=14.85 +/- 0.13 new_mean_mag=14.7554 delta=0.10 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:04:24.47 -14:09:22.3: 15.05 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.91 +/- 0.13
Forced photometry filter REJECTED candidate at 21:48:39.98 -12:10:46.3: ref_mag=14.91 +/- 0.13 new_mean_mag=14.6815 delta=0.23 (need > 0.90)
Forced photometry reference-image weighted average: 15.07 +/- 0.14
Forced photometry filter REJECTED candidate at 22:04:24.47 -14:09:22.3: ref_mag=15.07 +/- 0.14 new_mean_mag=14.7128 delta=0.36 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:55:01.63 -04:53:27.2: 15.06 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.92 +/- 0.12
Forced photometry filter REJECTED candidate at 21:55:01.63 -04:53:27.2: ref_mag=14.92 +/- 0.12 new_mean_mag=14.7248 delta=0.19 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:56:17.36 -13:15:05.3: 14.84 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.86 +/- 0.12
Forced photometry filter REJECTED candidate at 21:56:17.36 -13:15:05.3: ref_mag=14.86 +/- 0.12 new_mean_mag=14.6630 delta=0.19 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:45:25.11 -07:48:30.1: 15.11 +/- 0.24 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:53:09.83 -05:08:08.4: 14.76 +/- 0.15 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:46:26.38 -12:11:52.1: 15.06 +/- 0.23 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:48:03.00 -06:16:36.3: 14.61 +/- 0.14 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:07:01.89 -13:48:58.3: 15.13 +/- 0.20 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:45:25.11 -07:48:30.1: 14.76 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.88 +/- 0.14
Forced photometry filter REJECTED candidate at 22:45:25.11 -07:48:30.1: ref_mag=14.88 +/- 0.14 new_mean_mag=14.7441 delta=0.14 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:53:09.83 -05:08:08.4: 14.76 +/- 0.16 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:04:51.82 -14:28:58.9: 14.80 +/- 0.17 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:46:26.38 -12:11:52.1: 14.63 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.76 +/- 0.11
Forced photometry filter REJECTED candidate at 21:53:09.83 -05:08:08.4: ref_mag=14.76 +/- 0.11 new_mean_mag=14.7468 delta=0.01 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:48:03.00 -06:16:36.3: 14.85 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.76 +/- 0.13
Forced photometry filter REJECTED candidate at 21:46:26.38 -12:11:52.1: ref_mag=14.76 +/- 0.13 new_mean_mag=14.6279 delta=0.14 (need > 0.90)
Forced photometry reference-image weighted average: 14.70 +/- 0.11
Forced photometry filter REJECTED candidate at 21:48:03.00 -06:16:36.3: ref_mag=14.70 +/- 0.11 new_mean_mag=14.7079 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:07:01.89 -13:48:58.3: 14.97 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.04 +/- 0.13
Forced photometry filter REJECTED candidate at 22:07:01.89 -13:48:58.3: ref_mag=15.04 +/- 0.13 new_mean_mag=14.7005 delta=0.34 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:04:51.82 -14:28:58.9: 14.94 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.86 +/- 0.12
Forced photometry filter REJECTED candidate at 22:04:51.82 -14:28:58.9: ref_mag=14.86 +/- 0.12 new_mean_mag=14.6808 delta=0.18 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:49:26.41 -05:06:50.7: 14.78 +/- 0.16 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:42:30.23 -05:26:20.0: 15.18 +/- 0.23 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:53:12.56 -05:56:52.7: 15.06 +/- 0.20 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:38:14.55 -15:12:07.3: 14.45 +/- 0.15 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:46:44.38 -12:15:21.6: 15.03 +/- 0.22 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:49:26.41 -05:06:50.7: 15.08 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.89 +/- 0.13
Forced photometry filter REJECTED candidate at 21:49:26.41 -05:06:50.7: ref_mag=14.89 +/- 0.13 new_mean_mag=14.8020 delta=0.09 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:53:12.56 -05:56:52.7: 15.15 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.10 +/- 0.15
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:42:30.23 -05:26:20.0: 15.28 +/- 0.27 detection
Forced photometry filter REJECTED candidate at 21:53:12.56 -05:56:52.7: ref_mag=15.10 +/- 0.15 new_mean_mag=14.7468 delta=0.35 (need > 0.90)
Forced photometry reference-image weighted average: 15.22 +/- 0.17
Forced photometry filter REJECTED candidate at 22:42:30.23 -05:26:20.0: ref_mag=15.22 +/- 0.17 new_mean_mag=14.7307 delta=0.49 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:38:14.55 -15:12:07.3: 14.55 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.49 +/- 0.11
Forced photometry filter REJECTED candidate at 22:38:14.55 -15:12:07.3: ref_mag=14.49 +/- 0.11 new_mean_mag=14.6271 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:46:44.38 -12:15:21.6: 15.14 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.08 +/- 0.16
Forced photometry filter REJECTED candidate at 21:46:44.38 -12:15:21.6: ref_mag=15.08 +/- 0.16 new_mean_mag=14.6057 delta=0.47 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:54:31.18 -10:54:32.8: 15.29 +/- 0.24 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:54:31.11 -13:34:46.8: 15.11 +/- 0.23 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:54:31.18 -10:54:32.8: 15.34 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.32 +/- 0.17
Forced photometry filter REJECTED candidate at 21:54:31.18 -10:54:32.8: ref_mag=15.32 +/- 0.17 new_mean_mag=14.7085 delta=0.61 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:36:44.19 -14:21:35.4: 14.83 +/- 0.19 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:47:59.74 -13:11:43.3: 14.81 +/- 0.21 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:54:31.11 -13:34:46.8: 15.09 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.10 +/- 0.16
Forced photometry filter REJECTED candidate at 21:54:31.11 -13:34:46.8: ref_mag=15.10 +/- 0.16 new_mean_mag=14.7241 delta=0.38 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:36:44.19 -14:21:35.4: 14.47 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.60 +/- 0.11
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:47:59.74 -13:11:43.3: 15.03 +/- 0.27 detection
Forced photometry filter REJECTED candidate at 22:36:44.19 -14:21:35.4: ref_mag=14.60 +/- 0.11 new_mean_mag=14.5823 delta=0.02 (need > 0.90)
Forced photometry reference-image weighted average: 14.89 +/- 0.17
Forced photometry filter REJECTED candidate at 22:47:59.74 -13:11:43.3: ref_mag=14.89 +/- 0.17 new_mean_mag=14.6795 delta=0.21 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:43:52.99 -06:03:29.8: 15.18 +/- 0.25 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:01:35.18 -12:52:17.5: 15.19 +/- 0.22 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:48:25.34 -07:28:23.9: 15.05 +/- 0.23 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:52:19.07 -14:25:11.1: 14.64 +/- 0.16 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:43:52.99 -06:03:29.8: 14.88 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.99 +/- 0.15
Forced photometry filter REJECTED candidate at 22:43:52.99 -06:03:29.8: ref_mag=14.99 +/- 0.15 new_mean_mag=14.8070 delta=0.18 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:01:35.18 -12:52:17.5: 14.86 +/- 0.17 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:41:25.52 -11:55:11.7: 14.66 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.98 +/- 0.13
Forced photometry filter REJECTED candidate at 22:01:35.18 -12:52:17.5: ref_mag=14.98 +/- 0.13 new_mean_mag=14.7583 delta=0.22 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:35:24.15 -12:12:03.0: 15.43 +/- 0.28 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:48:25.34 -07:28:23.9: 14.92 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.98 +/- 0.16
Forced photometry filter REJECTED candidate at 22:48:25.34 -07:28:23.9: ref_mag=14.98 +/- 0.16 new_mean_mag=14.8269 delta=0.15 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:52:19.07 -14:25:11.1: 14.92 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.75 +/- 0.13
Forced photometry filter REJECTED candidate at 21:52:19.07 -14:25:11.1: ref_mag=14.75 +/- 0.13 new_mean_mag=14.5862 delta=0.16 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:41:25.52 -11:55:11.7: 14.69 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.68 +/- 0.11
Forced photometry filter REJECTED candidate at 22:41:25.52 -11:55:11.7: ref_mag=14.68 +/- 0.11 new_mean_mag=14.7123 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:35:24.15 -12:12:03.0: 15.26 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.33 +/- 0.18
Forced photometry filter REJECTED candidate at 22:35:24.15 -12:12:03.0: ref_mag=15.33 +/- 0.18 new_mean_mag=14.8105 delta=0.52 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:54:55.20 -14:27:13.1: 14.87 +/- 0.18 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:49:54.07 -14:33:15.2: 14.57 +/- 0.16 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:56:12.96 -09:01:55.9: 14.74 +/- 0.14 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:07:59.73 -13:03:43.9: 15.08 +/- 0.19 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:54:55.20 -14:27:13.1: 14.78 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.83 +/- 0.13
Forced photometry filter REJECTED candidate at 21:54:55.20 -14:27:13.1: ref_mag=14.83 +/- 0.13 new_mean_mag=14.5574 delta=0.27 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:49:54.07 -14:33:15.2: 14.88 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.69 +/- 0.12
Forced photometry filter REJECTED candidate at 21:49:54.07 -14:33:15.2: ref_mag=14.69 +/- 0.12 new_mean_mag=14.6378 delta=0.05 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:56:12.96 -09:01:55.9: 15.01 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.84 +/- 0.11
Forced photometry filter REJECTED candidate at 21:56:12.96 -09:01:55.9: ref_mag=14.84 +/- 0.11 new_mean_mag=14.6659 delta=0.18 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:07:59.73 -13:03:43.9: 15.15 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.11 +/- 0.14
Forced photometry filter REJECTED candidate at 22:07:59.73 -13:03:43.9: ref_mag=15.11 +/- 0.14 new_mean_mag=14.7730 delta=0.34 (need > 0.90)
Adding exclusion_list_local.txt__out53468.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53570.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53578.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 53395_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53395_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53397_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53397_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53403_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53403_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53428_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53428_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
**** FOUND 22:04:20.80 -14:35:23.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53468_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
Preparing report for the candidate 53468_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
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Considering the candidate 53514_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
Preparing report for the candidate 53514_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
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Considering the candidate 53570_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
Preparing report for the candidate 53570_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
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Considering the candidate 53578_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
Preparing report for the candidate 53578_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
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Considering the candidate 53715_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53715_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53716_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53716_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53729_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53729_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53736_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53736_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53762_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53762_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53769_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53769_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53772_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53772_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53790_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53790_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53794_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53794_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53801_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53801_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53803_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53803_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53807_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53807_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53811_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53811_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53812_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53812_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53814_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53814_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53820_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53820_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53822_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53822_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
**** FOUND 22:14:17.81 -12:38:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53824_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53824_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53833_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53833_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53834_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53834_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53835_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53835_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53836_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53836_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53856_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53856_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53857_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53857_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53859_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53859_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53860_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53860_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53861_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53861_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53862_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53862_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53866_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53866_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53867_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53867_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53868_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53868_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53869_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53869_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53875_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53875_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53876_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53876_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 53878_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53878_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53879_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53879_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53882_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53882_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53887_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53887_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53889_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53889_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53898_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53898_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53902_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53902_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53904_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53904_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53906_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53906_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53908_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53908_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53911_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53911_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53913_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53913_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53925_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53925_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 53930_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 53930_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
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Considering the candidate 12218_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181
The candidate 12218_fd_Aqr-04-Q1b1x1_2026-10-10_23-06-25_20.00sec_-0.00C_LIGHTs_0181 did not pass the final checks
