This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 07 09.2477 2461230.7477 11.24 20:58:41.72 -11:01:22.6
37.44108 -33.20957 galactic Aqr Second-epoch detections are separated by 0.6" and 11.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.287 Nephthys 0 -0 0 11.5 -0 -0
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 20:58:41.72 -11:01:22.6: 14.93 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 20:58:41.72 -11:01:22.6: 14.94 +/- 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,2461230.7477,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260709.2477 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 09.2477 2461230.7477 11.45 21:40:59.41 -10:04:25.9
44.35887 -42.10519 galactic Cap Second-epoch detections are separated by 0.4" and 10.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.306 Unitas -1 -0 1 11.4 0 -0
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:40:59.41 -10:04:25.9: 15.16 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:40:59.41 -10:04:25.9: 15.18 +/- 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 07 09.2477* 21 40 59.41 -10 04 25.9 11.4 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,2461230.7477,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260709.2477 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 09.2477 2461230.7477 11.74 21:42:59.05 -07:23:03.5
47.83344 -41.24362 galactic Aqr Second-epoch detections are separated by 0.5" and 10.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.389 Industria 0 0 0 12.2 0 0
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:42:59.05 -07:23:03.5: 15.12 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:42:59.05 -07:23:03.5: 15.15 +/- 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,2461230.7477,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260709.2477 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 09.2477 2461230.7477 13.58 21:39:38.42 -11:02:43.3
42.98819 -42.25412 galactic Cap Second-epoch detections are separated by 0.8" and 10.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.38 Leda -1 -1 1 13.4 -0 -0
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:39:38.42 -11:02:43.3: 15.17 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:39:38.42 -11:02:43.3: 15.15 +/- 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 07 09.2477* 21 39 38.42 -11 02 43.3 13.6 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,2461230.7477,13.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260709.2477 13.58CV 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: 2461177.87809874 17.05.2026 09:04:17.731 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
First image: 2461177.87809874 17.05.2026 09:04:17.731 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
Last image: 2461230.74801808 09.07.2026 05:56:58.762 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.20
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5737
Objects passed selection criteria: 5713
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 4153.5
Average stars matched: 4064 (97.8452 %)
Memory usage VmPeak: 112184 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 8 15:05:08 CDT 2026
VaST build number 1.0rc89-141-gc31ee76a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jul 9 01:03:46 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: 2461177.87809874 17.05.2026 09:04:17.731 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
First image: 2461177.87809874 17.05.2026 09:04:17.731 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
Last image: 2461230.74801808 09.07.2026 05:56:58.762 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 61
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.97
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: 11 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 29631
Objects passed selection criteria: 29598
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 25708.5
Average stars matched: 24891.2 (96.8211 %)
Memory usage VmPeak: 134404 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 8 15:05:08 CDT 2026
VaST build number 1.0rc89-141-gc31ee76a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jul 9 01:05:39 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
SExtractor catalog cache: saved Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat to cache
SExtractor catalog cache: saved Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.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-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461230.74745628
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-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits exists and is non-empty
Saving wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits to local_wcs_cache/
'wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits' -> 'local_wcs_cache/wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits'
wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits exists and is non-empty
Saving wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits to local_wcs_cache/
'wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits' -> 'local_wcs_cache/wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits'
wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits exists and is non-empty
Saving wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits to local_wcs_cache/
'wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits' -> 'local_wcs_cache/wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits'
wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits exists and is non-empty
Saving wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits to local_wcs_cache/
'wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits' -> 'local_wcs_cache/wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits (1st reference image)
verification OK: wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
Image size: 941.9'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: 21:25:33.187 -09:59:28.83 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-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits (1st new image)
verification OK: wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
Image size: 937.6'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:25:21.373 -09:59:40.69 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:25:33.187 -09:59:28.83
Second-epoch image center 21:25:21.373 -09:59:40.69
Angular distance between the image centers 0.0486 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits (2nd new image)
verification OK: wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
Image size: 937.6'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:25:24.359 -09:58:54.96 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:25:33.187 -09:59:28.83
Second-epoch image center 21:25:24.359 -09:58:54.96
Angular distance between the image centers 0.0374 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 21:25:21.373 -09:59:40.69
Second-epoch second image center 21:25:24.359 -09:58:54.96
Angular distance between the image centers 0.01765 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-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits &> /tmp/tmp.gPmfAiKPgI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits &> /tmp/tmp.PYq54KHkFG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits &> /tmp/tmp.BIajZL1GYL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits &> /tmp/tmp.8GTDFXA8JI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.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-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits and wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.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-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits and wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat
Found non-empty wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits and wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat
The reference image (wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits) and catalog (wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat) found
'wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat' -> 'wcsmag.cat'
Read 7159 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.0145 to 329.5552 deg, Dec -15.5597 to -4.2276 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 313.0145 to 329.5552 deg, Dec -15.5597 to -4.2276 deg
Loaded 7438 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): 5084 out of 5196 total matches.
Matched with Tycho-2 5196 out of 7159 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.636450
a=0.000000 b=1.000000 c=22.636450
From vast_summary.log: estimated ref. image limiting mag.: -8.20
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.44
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.44
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7159 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.0145 to 329.5552 deg, Dec -15.5597 to -4.2276 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 313.0145 to 329.5552 deg, Dec -15.5597 to -4.2276 deg
Loaded 7438 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): 5084 out of 5196 total matches.
Matched with Tycho-2 5196 out of 7159 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits:
Forced-photometry filter: calibrated wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits -> calib.txt_param_ref_wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits (aperture=7.3)
Read 7189 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.0145 to 329.5561 deg, Dec -15.5598 to -4.2276 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 313.0145 to 329.5561 deg, Dec -15.5598 to -4.2276 deg
Loaded 7439 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): 5086 out of 5190 total matches.
Matched with Tycho-2 5190 out of 7189 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits:
Forced-photometry filter: calibrated wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits -> calib.txt_param_ref_wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits (aperture=7.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
3.3 pix Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
3.3 pix Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
2.3 pix fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
2.3 pix fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
3.3 pix wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
3.3 pix wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
Limiting magnitude estimates:
14.4 mag. Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
14.4 mag. Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
13.6 mag. fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
13.6 mag. fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 10.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.gPmfAiKPgI (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.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-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits' -> 'wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
WCS_IMAGE_NAME=wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
WCS-calibrated image found: wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
Checking if the catalog wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat corresponding to the image wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits alredy exist and is non-empty...
Catalog wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat corresponding to the image wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
WCS catalog name: wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=329, bad_region=1230, passed=7159
Got 7159 stars (including 5649 good ones) from the SExtractor catalog wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat
util/solve_plate_with_UCAC5 got 7159 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 5961 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
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 5960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 5960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 943 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits N_match=943 sigma_overall_arcsec=0.273 sigma_q1_arcsec=0.304 sigma_q2_arcsec=0.276 sigma_q3_arcsec=0.228 sigma_q4_arcsec=0.256 n_q1=326 n_q2=154 n_q3=322 n_q4=141 worst_quadrant_to_overall_ratio=1.115
The image catalog is written to wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits -region wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.PYq54KHkFG (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.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-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits' -> 'wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
WCS_IMAGE_NAME=wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
WCS-calibrated image found: wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
Checking if the catalog wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat corresponding to the image wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits alredy exist and is non-empty...
Catalog wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat corresponding to the image wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
WCS catalog name: wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=325, bad_region=1224, passed=7189
Got 7189 stars (including 5692 good ones) from the SExtractor catalog wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat
util/solve_plate_with_UCAC5 got 7189 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5977 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
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 5977 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 5977 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 943 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits N_match=943 sigma_overall_arcsec=0.253 sigma_q1_arcsec=0.290 sigma_q2_arcsec=0.232 sigma_q3_arcsec=0.241 sigma_q4_arcsec=0.203 n_q1=333 n_q2=153 n_q3=316 n_q4=141 worst_quadrant_to_overall_ratio=1.148
The image catalog is written to wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits -region wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.BIajZL1GYL (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
WCS-calibrated image found: wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
Checking if the catalog wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
WCS catalog name: wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=200, bad_region=558, passed=2973
Got 2973 stars (including 2252 good ones) from the SExtractor catalog wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits.wcscat
util/solve_plate_with_UCAC5 got 2973 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 2446 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 2446 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 2446 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 942 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits N_match=942 sigma_overall_arcsec=0.388 sigma_q1_arcsec=0.382 sigma_q2_arcsec=0.362 sigma_q3_arcsec=0.421 sigma_q4_arcsec=0.399 n_q1=324 n_q2=169 n_q3=302 n_q4=147 worst_quadrant_to_overall_ratio=1.085
The image catalog is written to wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits -region wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.8GTDFXA8JI (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
WCS-calibrated image found: wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
Checking if the catalog wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
WCS catalog name: wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=221, bad_region=568, passed=2962
Got 2962 stars (including 2218 good ones) from the SExtractor catalog wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits.wcscat
util/solve_plate_with_UCAC5 got 2962 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 2430 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 2429 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 2429 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits N_match=943 sigma_overall_arcsec=0.407 sigma_q1_arcsec=0.406 sigma_q2_arcsec=0.372 sigma_q3_arcsec=0.449 sigma_q4_arcsec=0.445 n_q1=323 n_q2=168 n_q3=304 n_q4=148 worst_quadrant_to_overall_ratio=1.103
The image catalog is written to wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits -region wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits sigma_overall=0.273 worst_q_ratio=1.115
ref2=Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits sigma_overall=0.253 worst_q_ratio=1.148
new1=fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits sigma_overall=0.388 worst_q_ratio=1.085
new2=fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits sigma_overall=0.407 worst_q_ratio=1.103
reference average sigma_overall=0.263 worst_q_ratio=1.1315
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428_astrometric_residuals.png (943 matched stars from wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.24 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429_astrometric_residuals.png (943 matched stars from wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.22 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063_astrometric_residuals.png (942 matched stars from wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064_astrometric_residuals.png (943 matched stars from wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits'
Saving fully-calibrated image wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits'
Preparing the HTML report for the field Aqr-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:02:20.82 -09:40:08.2: 9.59 +/- 0.00 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:02:20.82 -09:40:08.2: 9.59 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.59 +/- 0.00
Forced photometry filter REJECTED candidate at 21:02:20.82 -09:40:08.2: ref_mag=9.59 +/- 0.00 new_mean_mag=10.3849 delta=-0.80 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20274_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 20274_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Aqr-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
SExtractor catalog cache: saved Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat to cache
SExtractor catalog cache: saved Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.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-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
Creating symlink local_wcs_cache/wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits exists and is non-empty
wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits exists and is non-empty
wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits exists and is non-empty
wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits (1st reference image)
verification OK: wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
Image size: 941.9'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: 21:25:33.187 -09:59:28.83 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-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits (1st new image)
verification OK: wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
Image size: 937.6'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:25:21.373 -09:59:40.69 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:25:33.187 -09:59:28.83
Second-epoch image center 21:25:21.373 -09:59:40.69
Angular distance between the image centers 0.0486 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits (2nd new image)
verification OK: wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
Image size: 937.6'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:25:24.359 -09:58:54.96 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:25:33.187 -09:59:28.83
Second-epoch image center 21:25:24.359 -09:58:54.96
Angular distance between the image centers 0.0374 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 21:25:21.373 -09:59:40.69
Second-epoch second image center 21:25:24.359 -09:58:54.96
Angular distance between the image centers 0.01765 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-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits &> /tmp/tmp.ZQAQGTx6n8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits &> /tmp/tmp.VnyVAY4qOu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits &> /tmp/tmp.QejVyHSH6p
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits &> /tmp/tmp.ouU2IOepNh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.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-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits and wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.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-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits and wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat
Found non-empty wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits and wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat
The reference image (wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits) and catalog (wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat) found
'wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat' -> 'wcsmag.cat'
Read 36787 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.0030 to 329.5641 deg, Dec -15.5697 to -4.2276 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 313.0030 to 329.5641 deg, Dec -15.5697 to -4.2276 deg
Loaded 7455 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): 5625 out of 6011 total matches.
Matched with Tycho-2 6011 out of 36787 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.510900
a=0.000000 b=1.000000 c=22.510900
From vast_summary.log: estimated ref. image limiting mag.: -7.97
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.54
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.54
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 36787 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.0030 to 329.5641 deg, Dec -15.5697 to -4.2276 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 313.0030 to 329.5641 deg, Dec -15.5697 to -4.2276 deg
Loaded 7455 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): 5625 out of 6011 total matches.
Matched with Tycho-2 6011 out of 36787 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits:
Forced-photometry filter: calibrated wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits -> calib.txt_param_ref_wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits (aperture=6.0)
Read 37049 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.0031 to 329.5643 deg, Dec -15.5699 to -4.2276 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 313.0031 to 329.5643 deg, Dec -15.5699 to -4.2276 deg
Loaded 7455 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): 5641 out of 6012 total matches.
Matched with Tycho-2 6012 out of 37049 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits:
Forced-photometry filter: calibrated wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits -> calib.txt_param_ref_wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 43 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
3.1 pix Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
3.1 pix Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
2.1 pix fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
2.1 pix fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
3.1 pix wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
3.1 pix wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
Limiting magnitude estimates:
14.5 mag. Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
14.5 mag. Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
13.8 mag. fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
13.8 mag. fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 13.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ZQAQGTx6n8 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.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-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits' -> 'wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
WCS_IMAGE_NAME=wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
WCS-calibrated image found: wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
Checking if the catalog wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat corresponding to the image wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits alredy exist and is non-empty...
Catalog wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat corresponding to the image wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
WCS catalog name: wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1449, bad_region=5274, passed=36781
Got 36781 stars (including 30184 good ones) from the SExtractor catalog wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat
util/solve_plate_with_UCAC5 got 36781 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 31650 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 31650 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 31650 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits N_match=942 sigma_overall_arcsec=0.283 sigma_q1_arcsec=0.307 sigma_q2_arcsec=0.271 sigma_q3_arcsec=0.247 sigma_q4_arcsec=0.274 n_q1=318 n_q2=147 n_q3=331 n_q4=146 worst_quadrant_to_overall_ratio=1.085
The image catalog is written to wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits -region wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.VnyVAY4qOu (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.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-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits' -> 'wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
WCS_IMAGE_NAME=wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
WCS-calibrated image found: wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
Checking if the catalog wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat corresponding to the image wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits alredy exist and is non-empty...
Catalog wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat corresponding to the image wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
WCS catalog name: wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1439, bad_region=5340, passed=37044
Got 37044 stars (including 30400 good ones) from the SExtractor catalog wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat
util/solve_plate_with_UCAC5 got 37044 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 31947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 31948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 31948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 946 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits N_match=946 sigma_overall_arcsec=0.277 sigma_q1_arcsec=0.304 sigma_q2_arcsec=0.261 sigma_q3_arcsec=0.256 sigma_q4_arcsec=0.244 n_q1=320 n_q2=152 n_q3=328 n_q4=146 worst_quadrant_to_overall_ratio=1.098
The image catalog is written to wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits -region wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.QejVyHSH6p (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
WCS-calibrated image found: wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
Checking if the catalog wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
WCS catalog name: wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=666, bad_region=2977, passed=23055
Got 23055 stars (including 19524 good ones) from the SExtractor catalog wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits.wcscat
util/solve_plate_with_UCAC5 got 23055 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 20180 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 20180 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 20180 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits N_match=943 sigma_overall_arcsec=0.395 sigma_q1_arcsec=0.388 sigma_q2_arcsec=0.339 sigma_q3_arcsec=0.429 sigma_q4_arcsec=0.396 n_q1=335 n_q2=162 n_q3=297 n_q4=149 worst_quadrant_to_overall_ratio=1.087
The image catalog is written to wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits -region wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ouU2IOepNh (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
WCS-calibrated image found: wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
Checking if the catalog wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
WCS catalog name: wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=671, bad_region=2964, passed=23211
Got 23211 stars (including 19688 good ones) from the SExtractor catalog wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits.wcscat
util/solve_plate_with_UCAC5 got 23211 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 20423 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 20422 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 20422 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits N_match=943 sigma_overall_arcsec=0.388 sigma_q1_arcsec=0.378 sigma_q2_arcsec=0.328 sigma_q3_arcsec=0.445 sigma_q4_arcsec=0.398 n_q1=332 n_q2=163 n_q3=297 n_q4=151 worst_quadrant_to_overall_ratio=1.147
The image catalog is written to wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits -region wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-10_20.00sec_-0.00C_LIGHT_0063.fits
Saving fully-calibrated image wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Aqr-03-Q2b1x1_010132_TTUQ2b1x1_3672278_bYhGAKk3/wcs_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064.fits
Preparing the HTML report for the field Aqr-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:38:57.98 -08:15:42.6: 12.78 +/- 0.04 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:11:19.30 -10:16:41.8: 12.57 +/- 0.03 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:17:23.56 -10:32:58.1: 12.16 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:25:12.36 -09:58:16.3: 12.67 +/- 0.03 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:13:14.41 -11:43:02.9: 12.39 +/- 0.03 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:26:01.94 -08:18:53.8: 12.78 +/- 0.04 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:31:59.19 -08:46:35.7: 13.00 +/- 0.05 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:36:09.72 -06:01:22.3: 11.96 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:25:43.57 -07:09:09.2: 12.13 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 20:59:44.54 -07:17:10.2: 11.94 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:25:12.36 -09:58:16.3: 12.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.02
Forced photometry filter REJECTED candidate at 21:25:12.36 -09:58:16.3: ref_mag=12.72 +/- 0.02 new_mean_mag=12.9791 delta=-0.26 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:38:57.98 -08:15:42.6: 12.82 +/- 0.04 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:25:43.57 -07:09:09.2: 12.20 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:31:59.19 -08:46:35.7: 13.01 +/- 0.05 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:13:14.41 -11:43:02.9: 12.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.03
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:26:01.94 -08:18:53.8: 12.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.01
Forced photometry filter REJECTED candidate at 21:38:57.98 -08:15:42.6: ref_mag=12.80 +/- 0.03 new_mean_mag=13.0935 delta=-0.29 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:25:43.57 -07:09:09.2: ref_mag=12.16 +/- 0.01 new_mean_mag=12.6566 delta=-0.49 (need > 0.90)
Forced photometry reference-image weighted average: 13.00 +/- 0.03
Forced photometry reference-image weighted average: 12.43 +/- 0.02
Forced photometry filter REJECTED candidate at 21:31:59.19 -08:46:35.7: ref_mag=13.00 +/- 0.03 new_mean_mag=13.4460 delta=-0.44 (need > 0.90)
Forced photometry reference-image weighted average: 12.77 +/- 0.03
Forced photometry filter REJECTED candidate at 21:13:14.41 -11:43:02.9: ref_mag=12.43 +/- 0.02 new_mean_mag=12.8338 delta=-0.41 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:26:01.94 -08:18:53.8: ref_mag=12.77 +/- 0.03 new_mean_mag=13.6817 delta=-0.91 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 20:59:44.54 -07:17:10.2: 11.97 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:17:23.56 -10:32:58.1: 12.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.95 +/- 0.02
Forced photometry filter REJECTED candidate at 20:59:44.54 -07:17:10.2: ref_mag=11.95 +/- 0.02 new_mean_mag=12.4949 delta=-0.54 (need > 0.90)
Forced photometry reference-image weighted average: 12.16 +/- 0.02
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:11:19.30 -10:16:41.8: 12.63 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 21:17:23.56 -10:32:58.1: ref_mag=12.16 +/- 0.02 new_mean_mag=12.7382 delta=-0.58 (need > 0.90)
Forced photometry reference-image weighted average: 12.60 +/- 0.02
Forced photometry filter REJECTED candidate at 21:11:19.30 -10:16:41.8: ref_mag=12.60 +/- 0.02 new_mean_mag=12.8932 delta=-0.29 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:36:09.72 -06:01:22.3: 11.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.95 +/- 0.01
Forced photometry filter REJECTED candidate at 21:36:09.72 -06:01:22.3: ref_mag=11.95 +/- 0.01 new_mean_mag=12.4549 delta=-0.51 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:04:59.99 -09:17:35.1: 12.03 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:16:51.50 -10:58:32.7: 11.69 +/- 0.01 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 20:58:53.36 -12:37:54.8: 11.83 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:00:40.05 -08:43:52.9: 11.54 +/- 0.01 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:07:54.63 -07:25:02.0: 10.31 +/- 0.00 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:32:40.54 -14:12:20.9: 11.89 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:35:32.55 -11:46:55.2: 10.78 +/- 0.01 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:02:20.81 -09:40:08.3: 9.77 +/- 0.00 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:05:12.27 -10:18:32.9: 11.11 +/- 0.01 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:04:59.99 -09:17:35.1: 12.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.04 +/- 0.02
Forced photometry filter REJECTED candidate at 21:04:59.99 -09:17:35.1: ref_mag=12.04 +/- 0.02 new_mean_mag=12.2866 delta=-0.25 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:00:40.05 -08:43:52.9: 11.57 +/- 0.01 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 20:58:53.36 -12:37:54.8: 11.85 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:07:54.63 -07:25:02.0: 10.31 +/- 0.00 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:16:51.50 -10:58:32.7: 11.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.31 +/- 0.00
Forced photometry reference-image weighted average: 11.55 +/- 0.01
Forced photometry reference-image weighted average: 11.84 +/- 0.02
Forced photometry filter REJECTED candidate at 21:00:40.05 -08:43:52.9: ref_mag=11.55 +/- 0.01 new_mean_mag=11.5252 delta=0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:07:54.63 -07:25:02.0: ref_mag=10.31 +/- 0.00 new_mean_mag=10.6858 delta=-0.37 (need > 0.90)
Forced photometry filter REJECTED candidate at 20:58:53.36 -12:37:54.8: ref_mag=11.84 +/- 0.02 new_mean_mag=12.1718 delta=-0.33 (need > 0.90)
Forced photometry reference-image weighted average: 11.71 +/- 0.01
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:32:40.54 -14:12:20.9: 11.95 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:05:12.27 -10:18:32.9: 11.09 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 21:16:51.50 -10:58:32.7: ref_mag=11.71 +/- 0.01 new_mean_mag=12.3256 delta=-0.62 (need > 0.90)
Forced photometry reference-image weighted average: 11.91 +/- 0.01
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:35:32.55 -11:46:55.2: 10.75 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.10 +/- 0.01
Forced photometry filter REJECTED candidate at 21:32:40.54 -14:12:20.9: ref_mag=11.91 +/- 0.01 new_mean_mag=12.4082 delta=-0.49 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:05:12.27 -10:18:32.9: ref_mag=11.10 +/- 0.01 new_mean_mag=11.1711 delta=-0.07 (need > 0.90)
Forced photometry reference-image weighted average: 10.76 +/- 0.00
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:20:14.57 -06:48:49.6: 11.86 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 21:35:32.55 -11:46:55.2: ref_mag=10.76 +/- 0.00 new_mean_mag=11.0320 delta=-0.27 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:02:20.81 -09:40:08.3: 9.78 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.77 +/- 0.00
Forced photometry filter REJECTED candidate at 21:02:20.81 -09:40:08.3: ref_mag=9.77 +/- 0.00 new_mean_mag=10.3079 delta=-0.53 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:20:14.57 -06:48:49.6: 11.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.84 +/- 0.01
Forced photometry filter REJECTED candidate at 21:20:14.57 -06:48:49.6: ref_mag=11.84 +/- 0.01 new_mean_mag=12.2966 delta=-0.46 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 20:58:41.72 -11:01:22.6: 14.93 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:40:59.41 -10:04:25.9: 15.16 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:34:41.10 -08:57:01.4: 11.67 +/- 0.01 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 20:58:05.13 -13:09:42.5: 11.55 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:42:59.05 -07:23:03.5: 15.12 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:17:41.87 -08:51:55.9: 11.79 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:19:43.82 -08:46:29.0: 11.51 +/- 0.01 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:21:25.14 -06:19:50.5: 11.58 +/- 0.01 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:29:52.53 -14:13:00.5: 12.02 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 20:58:41.72 -11:01:22.6: 14.94 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:40:59.41 -10:04:25.9: 15.18 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:34:41.10 -08:57:01.4: 11.75 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:42:59.05 -07:23:03.5: 15.15 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 11.70 +/- 0.01
Forced photometry filter REJECTED candidate at 21:34:41.10 -08:57:01.4: ref_mag=11.70 +/- 0.01 new_mean_mag=12.0435 delta=-0.34 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 20:58:05.13 -13:09:42.5: 11.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.58 +/- 0.01
Forced photometry filter REJECTED candidate at 20:58:05.13 -13:09:42.5: ref_mag=11.58 +/- 0.01 new_mean_mag=11.8423 delta=-0.26 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:17:41.87 -08:51:55.9: 11.78 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:20:15.01 -10:48:45.4: 12.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.79 +/- 0.01
Forced photometry filter REJECTED candidate at 21:17:41.87 -08:51:55.9: ref_mag=11.79 +/- 0.01 new_mean_mag=12.0753 delta=-0.29 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:19:43.82 -08:46:29.0: 11.51 +/- 0.01 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:21:25.14 -06:19:50.5: 11.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.51 +/- 0.01
Forced photometry filter REJECTED candidate at 21:19:43.82 -08:46:29.0: ref_mag=11.51 +/- 0.01 new_mean_mag=12.0590 delta=-0.55 (need > 0.90)
Forced photometry reference-image weighted average: 11.59 +/- 0.01
Forced photometry filter REJECTED candidate at 21:21:25.14 -06:19:50.5: ref_mag=11.59 +/- 0.01 new_mean_mag=12.2501 delta=-0.66 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:29:52.53 -14:13:00.5: 12.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.03 +/- 0.02
Forced photometry filter REJECTED candidate at 21:29:52.53 -14:13:00.5: ref_mag=12.03 +/- 0.02 new_mean_mag=12.4559 delta=-0.42 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:20:15.01 -10:48:45.4: 12.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.02
Forced photometry filter REJECTED candidate at 21:20:15.01 -10:48:45.4: ref_mag=12.25 +/- 0.02 new_mean_mag=12.3959 delta=-0.15 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:00:01.07 -13:24:30.1: 12.24 +/- 0.03 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:12:23.28 -10:52:12.0: 12.17 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:10:02.64 -11:30:50.0: 12.81 +/- 0.04 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:04:16.29 -06:21:03.4: 12.10 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:08:34.48 -06:47:43.2: 11.92 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:05:27.87 -12:17:32.7: 12.34 +/- 0.03 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:00:01.07 -13:24:30.1: 12.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.02
Forced photometry filter REJECTED candidate at 21:00:01.07 -13:24:30.1: ref_mag=12.21 +/- 0.02 new_mean_mag=12.4917 delta=-0.28 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:12:23.28 -10:52:12.0: 12.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.15 +/- 0.02
Forced photometry filter REJECTED candidate at 21:12:23.28 -10:52:12.0: ref_mag=12.15 +/- 0.02 new_mean_mag=12.5145 delta=-0.36 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:42:02.30 -06:00:09.8: 12.52 +/- 0.03 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:10:02.64 -11:30:50.0: 12.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.03
Forced photometry filter REJECTED candidate at 21:10:02.64 -11:30:50.0: ref_mag=12.84 +/- 0.03 new_mean_mag=12.7697 delta=0.07 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:04:16.29 -06:21:03.4: 12.18 +/- 0.03 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:08:34.48 -06:47:43.2: 11.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.02
Forced photometry reference-image weighted average: 11.93 +/- 0.01
Forced photometry filter REJECTED candidate at 21:04:16.29 -06:21:03.4: ref_mag=12.14 +/- 0.02 new_mean_mag=12.5014 delta=-0.36 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:08:34.48 -06:47:43.2: ref_mag=11.93 +/- 0.01 new_mean_mag=12.6788 delta=-0.74 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:05:27.87 -12:17:32.7: 12.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.02
Forced photometry filter REJECTED candidate at 21:05:27.87 -12:17:32.7: ref_mag=12.34 +/- 0.02 new_mean_mag=12.8346 delta=-0.49 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:42:02.30 -06:00:09.8: 12.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.02
Forced photometry filter REJECTED candidate at 21:42:02.30 -06:00:09.8: ref_mag=12.49 +/- 0.02 new_mean_mag=12.9211 delta=-0.43 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:02:22.13 -09:41:24.5: 13.15 +/- 0.07 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:31:33.95 -10:10:37.2: 12.62 +/- 0.03 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:40:17.84 -08:12:21.8: 12.73 +/- 0.04 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:19:23.97 -12:30:14.0: 12.60 +/- 0.04 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:22:25.37 -08:26:38.3: 13.04 +/- 0.05 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:39:38.42 -11:02:43.3: 15.17 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:31:33.95 -10:10:37.2: 12.65 +/- 0.03 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:02:22.13 -09:41:24.5: 13.02 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.02
Forced photometry filter REJECTED candidate at 21:31:33.95 -10:10:37.2: ref_mag=12.63 +/- 0.02 new_mean_mag=12.9659 delta=-0.33 (need > 0.90)
Forced photometry reference-image weighted average: 13.08 +/- 0.04
Forced photometry filter REJECTED candidate at 21:02:22.13 -09:41:24.5: ref_mag=13.08 +/- 0.04 new_mean_mag=12.9706 delta=0.11 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:40:17.84 -08:12:21.8: 12.63 +/- 0.03 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:22:25.37 -08:26:38.3: 13.00 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.03
Forced photometry reference-image weighted average: 13.02 +/- 0.03
Forced photometry filter REJECTED candidate at 21:40:17.84 -08:12:21.8: ref_mag=12.68 +/- 0.03 new_mean_mag=13.0599 delta=-0.38 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:22:25.37 -08:26:38.3: ref_mag=13.02 +/- 0.03 new_mean_mag=13.3265 delta=-0.31 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:19:23.97 -12:30:14.0: 12.59 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.02
Forced photometry filter REJECTED candidate at 21:19:23.97 -12:30:14.0: ref_mag=12.59 +/- 0.02 new_mean_mag=13.1523 delta=-0.56 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:39:38.42 -11:02:43.3: 15.15 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out52686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52690.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53118.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 52551_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52551_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52556_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52556_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52563_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52563_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52566_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52566_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52569_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52569_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52570_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52570_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52571_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52571_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52572_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52572_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52574_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52574_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52575_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52575_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52576_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52576_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52577_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52577_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52578_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52578_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52579_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52579_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52580_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52580_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52581_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52581_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52582_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52582_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52583_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52583_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52653_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52653_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52671_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52671_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52686_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
Preparing report for the candidate 52686_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
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Considering the candidate 52690_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
Preparing report for the candidate 52690_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
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Considering the candidate 52720_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
Preparing report for the candidate 52720_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
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Considering the candidate 52737_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52737_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52743_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52743_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52750_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52750_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52755_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52755_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52797_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52797_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52809_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52809_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52821_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52821_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52863_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52863_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52904_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52904_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52913_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52913_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52926_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52926_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52927_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52927_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52941_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52941_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52959_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52959_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52989_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52989_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 52991_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 52991_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 53036_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 53036_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 53057_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 53057_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks
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Considering the candidate 53087_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064
The candidate 53087_fd_Aqr-03-Q2b1x1_2026-07-09_00-56-58_20.00sec_-0.00C_LIGHT_0064 did not pass the final checks