This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK
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 08 18.2833 2461270.7833 14.13 22:05:28.03 -00:00:11.3
60.20098 -41.80995 galactic Aqr Second-epoch detections are separated by 1.9" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.607 Jenny -0 -0 0 14.1 -0 -0
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:05:28.03 -00:00:11.3: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:05:28.03 -00:00:11.3: 15.87 +/- 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,2461270.7833,14.13,0.05,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 20260818.2833 14.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 18.2833 2461270.7833 14.30 22:14:28.68 +02:03:47.7
64.27258 -42.25529 galactic Aqr Second-epoch detections are separated by 2.3" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1547 Nele 0 1 1 14.5 -0 -0
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:14:28.68 +02:03:47.7: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:14:28.68 +02:03:47.7: 15.92 +/- 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,2461270.7833,14.30,0.05,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 20260818.2833 14.30CV 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 08 18.2833 2461270.7833 14.43 22:00:18.13 -03:10:19.1
55.71830 -42.64163 galactic Aqr Second-epoch detections are separated by 0.9" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.2141 Simferopol 1 -1 1 14.8 -0 0
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:00:18.13 -03:10:19.1: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:00:18.13 -03:10:19.1: 15.90 +/- 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,2461270.7833,14.43,0.05,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 20260818.2833 14.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 18.2833 2461270.7833 13.62 22:14:07.92 -04:41:15.4
56.74982 -46.33670 galactic Aqr Second-epoch detections are separated by 0.8" and 9.0 pix
The object was found in VSX 1" NSVS 14496660
Type: RRAB
# Max. Min./Amp. JD0 Period
14.255 CV Y 1.030 CV 2455334.15960 0.487326100000
The object was not found in astcheck.
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:14:07.92 -04:41:15.4: 14.64 +/- 0.13 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:14:07.92 -04:41:15.4: 14.81 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.71 +/- 0.09
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
NSVS 14496660,2461270.7833,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 14496660 20260818.2833 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461242.93295420 21.07.2026 10:23:17.243 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
First image: 2461242.93295420 21.07.2026 10:23:17.243 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Last image: 2461270.78360946 18.08.2026 06:48:13.857 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.55
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: 5 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 7330
Objects passed selection criteria: 7309
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 5684.5
Average stars matched: 5065.5 (89.1107 %)
Memory usage VmPeak: 233016 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Aug 14 19:27:11 CDT 2026
VaST build number 1.0rc89-191-g1c132b07
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Aug 18 01:57:39 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461242.93295420 21.07.2026 10:23:17.243 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
First image: 2461242.93295420 21.07.2026 10:23:17.243 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Last image: 2461270.78360946 18.08.2026 06:48:13.857 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 47
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.24
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: 39 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 45493
Objects passed selection criteria: 45332
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 37075
Average stars matched: 33060.8 (89.1726 %)
Memory usage VmPeak: 263388 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Aug 14 19:27:11 CDT 2026
VaST build number 1.0rc89-191-g1c132b07
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Aug 18 01:59:13 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
SExtractor catalog cache: saved Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.cat to cache
SExtractor catalog cache: saved Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.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-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.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: 2461270.78299103
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-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits exists and is non-empty
wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits exists and is non-empty
wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits exists and is non-empty
wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits (1st reference image)
verification OK: wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Image size: 937.5'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:09.355 -02:00:05.25 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits (1st new image)
verification OK: wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:08.613 -01:59:23.08 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:17:09.355 -02:00:05.25
Second-epoch image center 22:17:08.613 -01:59:23.08
Angular distance between the image centers 0.0121 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits (2nd new image)
verification OK: wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:11.583 -01:59:52.09 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:17:09.355 -02:00:05.25
Second-epoch image center 22:17:11.583 -01:59:52.09
Angular distance between the image centers 0.0100 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 22:17:08.613 -01:59:23.08
Second-epoch second image center 22:17:11.583 -01:59:52.09
Angular distance between the image centers 0.01476 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-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits &> /tmp/tmp.ZKUTaa7fVM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits &> /tmp/tmp.ebvQ23u0Th
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits &> /tmp/tmp.QrvUqxCIn0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits &> /tmp/tmp.hUidlcAZ8f
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.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-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits and wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.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-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits and wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat
Found non-empty wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits and wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat
The reference image (wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits) and catalog (wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat) found
'wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat' -> 'wcsmag.cat'
Read 7776 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.4297 to 342.1786 deg, Dec -7.2616 to +3.2651 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 326.4297 to 342.1786 deg, Dec -7.2616 to 3.2651 deg
Loaded 5154 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): 4414 out of 4557 total matches.
Matched with Tycho-2 4557 out of 7776 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.628200
a=0.000000 b=1.000000 c=22.628200
From vast_summary.log: estimated ref. image limiting mag.: -7.55
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.08
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.08
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7776 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.4297 to 342.1786 deg, Dec -7.2616 to +3.2651 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 326.4297 to 342.1786 deg, Dec -7.2616 to 3.2651 deg
Loaded 5154 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): 4414 out of 4557 total matches.
Matched with Tycho-2 4557 out of 7776 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Forced-photometry filter: calibrated wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits -> calib.txt_param_ref_wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits (aperture=6.2)
Read 7733 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.4352 to 342.1813 deg, Dec -7.2521 to +3.2799 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 326.4352 to 342.1813 deg, Dec -7.2521 to 3.2799 deg
Loaded 5154 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): 4402 out of 4552 total matches.
Matched with Tycho-2 4552 out of 7733 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
Forced-photometry filter: calibrated wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits -> calib.txt_param_ref_wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits (aperture=6.2)
____ 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:
2.3 pix Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
2.3 pix Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
2.3 pix fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits
2.3 pix fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
Limiting magnitude estimates:
15.1 mag. Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
15.1 mag. Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
15.0 mag. fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits
15.0 mag. fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.ZKUTaa7fVM (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.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-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits' -> 'wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
WCS_IMAGE_NAME=wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
WCS-calibrated image found: wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Checking if the catalog wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat corresponding to the image wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits alredy exist and is non-empty...
Catalog wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat corresponding to the image wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
WCS catalog name: wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.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=420, bad_region=2142, passed=7776
Got 7776 stars (including 5312 good ones) from the SExtractor catalog wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat
util/solve_plate_with_UCAC5 got 7776 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4530 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4509 matched stars entering correct_measured_positions(), 4509 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4509 matched stars entering correct_measured_positions(), 6065 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4529 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4508 matched stars entering correct_measured_positions(), 6065 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4508 matched stars entering correct_measured_positions(), 6065 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4508 stars left (next iteration limit 4959)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits N_match=4508 sigma_overall_arcsec=0.379 sigma_q1_arcsec=0.360 sigma_q2_arcsec=0.385 sigma_q3_arcsec=0.374 sigma_q4_arcsec=0.338 n_q1=1393 n_q2=902 n_q3=1359 n_q4=854 worst_quadrant_to_overall_ratio=1.017
The image catalog is written to wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits -region wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.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.ebvQ23u0Th (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.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-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits' -> 'wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
WCS_IMAGE_NAME=wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
WCS-calibrated image found: wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
Checking if the catalog wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat corresponding to the image wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits alredy exist and is non-empty...
Catalog wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat corresponding to the image wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
WCS catalog name: wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.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=446, bad_region=2127, passed=7733
Got 7733 stars (including 5260 good ones) from the SExtractor catalog wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat
util/solve_plate_with_UCAC5 got 7733 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4539 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4515 matched stars entering correct_measured_positions(), 4515 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4515 matched stars entering correct_measured_positions(), 6014 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4539 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4514 matched stars entering correct_measured_positions(), 6014 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4514 matched stars entering correct_measured_positions(), 6014 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4514 stars left (next iteration limit 4966)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits N_match=4514 sigma_overall_arcsec=0.418 sigma_q1_arcsec=0.380 sigma_q2_arcsec=0.433 sigma_q3_arcsec=0.430 sigma_q4_arcsec=0.411 n_q1=1390 n_q2=906 n_q3=1375 n_q4=843 worst_quadrant_to_overall_ratio=1.038
The image catalog is written to wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits -region wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.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.QrvUqxCIn0 (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_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.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_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits
WCS-calibrated image found: wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits
Checking if the catalog wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits.wcscat corresponding to the image wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits.wcscat corresponding to the image wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits
WCS catalog name: wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=492, bad_region=1596, passed=7442
Got 7442 stars (including 5446 good ones) from the SExtractor catalog wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits.wcscat
util/solve_plate_with_UCAC5 got 7442 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4638 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4617 matched stars entering correct_measured_positions(), 4618 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4617 matched stars entering correct_measured_positions(), 6174 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4639 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4618 matched stars entering correct_measured_positions(), 6174 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 4618 matched stars entering correct_measured_positions(), 6174 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4618 stars left (next iteration limit 5078)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4618 robust_rms=6.537 arcsec worst_quadrant_rms=11.876 arcsec
SIP_REFIT: SIP order 3 trial: matched=4618 robust_rms=0.586 arcsec worst_quadrant_rms=0.719 arcsec
SIP_REFIT: SIP order 5 trial: matched=4618 robust_rms=0.409 arcsec worst_quadrant_rms=0.458 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4618 robust_rms_before=0.910 arcsec robust_rms_before_corrected=0.428 arcsec robust_rms_after=0.409 arcsec worst_quadrant_rms_before=0.474 worst_quadrant_rms_after=0.458
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.474 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits N_match=4618 sigma_overall_arcsec=0.449 sigma_q1_arcsec=0.378 sigma_q2_arcsec=0.443 sigma_q3_arcsec=0.514 sigma_q4_arcsec=0.423 n_q1=1545 n_q2=699 n_q3=1561 n_q4=813 worst_quadrant_to_overall_ratio=1.143
The image catalog is written to wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits -region wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.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.hUidlcAZ8f (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_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.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_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
WCS-calibrated image found: wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
Checking if the catalog wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits.wcscat corresponding to the image wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits.wcscat corresponding to the image wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
WCS catalog name: wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.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=489, bad_region=1590, passed=7410
Got 7410 stars (including 5427 good ones) from the SExtractor catalog wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits.wcscat
util/solve_plate_with_UCAC5 got 7410 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4633 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4613 matched stars entering correct_measured_positions(), 4614 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4613 matched stars entering correct_measured_positions(), 6148 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4634 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4613 matched stars entering correct_measured_positions(), 6148 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 4613 matched stars entering correct_measured_positions(), 6148 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 4613 stars left (next iteration limit 5074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4613 robust_rms=6.403 arcsec worst_quadrant_rms=12.304 arcsec
SIP_REFIT: SIP order 3 trial: matched=4613 robust_rms=0.572 arcsec worst_quadrant_rms=0.715 arcsec
SIP_REFIT: SIP order 5 trial: matched=4613 robust_rms=0.397 arcsec worst_quadrant_rms=0.438 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4613 robust_rms_before=0.909 arcsec robust_rms_before_corrected=0.416 arcsec robust_rms_after=0.397 arcsec worst_quadrant_rms_before=0.459 worst_quadrant_rms_after=0.438
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.459 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits N_match=4613 sigma_overall_arcsec=0.435 sigma_q1_arcsec=0.367 sigma_q2_arcsec=0.432 sigma_q3_arcsec=0.486 sigma_q4_arcsec=0.406 n_q1=1555 n_q2=689 n_q3=1564 n_q4=805 worst_quadrant_to_overall_ratio=1.117
The image catalog is written to wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits -region wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Saving the final (post-refit) wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits to local_wcs_cache/
'wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits' -> 'local_wcs_cache/wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits'
Saving the final (post-refit) wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits to local_wcs_cache/
'wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits' -> 'local_wcs_cache/wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits'
Saving the final (post-refit) wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits to local_wcs_cache/
'wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits' -> 'local_wcs_cache/wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits'
Saving the final (post-refit) wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits to local_wcs_cache/
'wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits' -> 'local_wcs_cache/wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits sigma_overall=0.379 worst_q_ratio=1.017
ref2=Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits sigma_overall=0.418 worst_q_ratio=1.038
new1=fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits sigma_overall=0.449 worst_q_ratio=1.143
new2=fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits sigma_overall=0.435 worst_q_ratio=1.117
reference average sigma_overall=0.3985 worst_q_ratio=1.0275
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013_astrometric_residuals.png (4508 matched stars from wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014_astrometric_residuals.png (4514 matched stars from wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288_astrometric_residuals.png (4618 matched stars from wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.38 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289_astrometric_residuals.png (4613 matched stars from wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.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-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits'
Saving fully-calibrated image wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits'
Preparing the HTML report for the field Aqr-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:16:34.96 -03:48:55.4: 12.52 +/- 0.02 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:16:34.96 -03:48:55.4: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Forced photometry filter REJECTED candidate at 22:16:34.96 -03:48:55.4: ref_mag=12.54 +/- 0.01 new_mean_mag=11.8506 delta=0.69 (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: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21492_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 21492_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Aqr-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
SExtractor catalog cache: saved Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.cat to cache
SExtractor catalog cache: saved Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.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-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Creating symlink local_wcs_cache/wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
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-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits exists and is non-empty
wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits exists and is non-empty
wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits exists and is non-empty
wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits (1st reference image)
verification OK: wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Image size: 937.5'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:09.355 -02:00:05.25 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits (1st new image)
verification OK: wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:08.613 -01:59:23.08 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:17:09.355 -02:00:05.25
Second-epoch image center 22:17:08.613 -01:59:23.08
Angular distance between the image centers 0.0121 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits (2nd new image)
verification OK: wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:11.583 -01:59:52.09 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:17:09.355 -02:00:05.25
Second-epoch image center 22:17:11.583 -01:59:52.09
Angular distance between the image centers 0.0100 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 22:17:08.613 -01:59:23.08
Second-epoch second image center 22:17:11.583 -01:59:52.09
Angular distance between the image centers 0.01476 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-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits &> /tmp/tmp.YnVAy1yOVh
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits &> /tmp/tmp.AXW3ldPQWH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits &> /tmp/tmp.btVMTNe6M0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits &> /tmp/tmp.5yRlPA3CA4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.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-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits and wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.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-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits and wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat
Found non-empty wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits and wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat
The reference image (wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits) and catalog (wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat) found
'wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat' -> 'wcsmag.cat'
Read 46863 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.4298 to 342.1802 deg, Dec -7.2660 to +3.2673 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 326.4298 to 342.1802 deg, Dec -7.2660 to 3.2673 deg
Loaded 5156 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): 4240 out of 4650 total matches.
Matched with Tycho-2 4650 out of 46863 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.491650
a=0.000000 b=1.000000 c=22.491650
From vast_summary.log: estimated ref. image limiting mag.: -7.24
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.25
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.25
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 46863 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.4298 to 342.1802 deg, Dec -7.2660 to +3.2673 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 326.4298 to 342.1802 deg, Dec -7.2660 to 3.2673 deg
Loaded 5156 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): 4240 out of 4650 total matches.
Matched with Tycho-2 4650 out of 46863 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Forced-photometry filter: calibrated wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits -> calib.txt_param_ref_wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits (aperture=4.7)
Read 47307 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.4340 to 342.1839 deg, Dec -7.2541 to +3.2809 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 326.4340 to 342.1839 deg, Dec -7.2541 to 3.2809 deg
Loaded 5159 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): 4244 out of 4656 total matches.
Matched with Tycho-2 4656 out of 47307 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
Forced-photometry filter: calibrated wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits -> calib.txt_param_ref_wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 37 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
2.1 pix Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
2.1 pix fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits
2.1 pix fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
Limiting magnitude estimates:
15.3 mag. Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
15.2 mag. Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
15.2 mag. fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits
15.2 mag. fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 14.6 (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.YnVAy1yOVh (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.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-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits' -> 'wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
WCS_IMAGE_NAME=wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
WCS-calibrated image found: wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Checking if the catalog wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat corresponding to the image wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits alredy exist and is non-empty...
Catalog wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat corresponding to the image wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
WCS catalog name: wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=2071, bad_region=10220, passed=46844
Got 46844 stars (including 35017 good ones) from the SExtractor catalog wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat
util/solve_plate_with_UCAC5 got 46844 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4525 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4507 matched stars entering correct_measured_positions(), 4507 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4507 matched stars entering correct_measured_positions(), 39065 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4525 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4507 matched stars entering correct_measured_positions(), 39065 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4507 matched stars entering correct_measured_positions(), 39065 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4507 stars left (next iteration limit 4957)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits N_match=4507 sigma_overall_arcsec=0.361 sigma_q1_arcsec=0.356 sigma_q2_arcsec=0.371 sigma_q3_arcsec=0.366 sigma_q4_arcsec=0.325 n_q1=1375 n_q2=933 n_q3=1339 n_q4=860 worst_quadrant_to_overall_ratio=1.028
The image catalog is written to wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits -region wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.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.AXW3ldPQWH (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.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-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits' -> 'wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
WCS_IMAGE_NAME=wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
WCS-calibrated image found: wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
Checking if the catalog wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat corresponding to the image wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits alredy exist and is non-empty...
Catalog wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat corresponding to the image wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
WCS catalog name: wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.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=15, blended=2102, bad_region=10366, passed=47292
Got 47292 stars (including 35288 good ones) from the SExtractor catalog wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat
util/solve_plate_with_UCAC5 got 47292 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4526 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4507 matched stars entering correct_measured_positions(), 4507 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4507 matched stars entering correct_measured_positions(), 39363 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4526 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4507 matched stars entering correct_measured_positions(), 39363 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4507 matched stars entering correct_measured_positions(), 39363 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4507 stars left (next iteration limit 4957)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits N_match=4507 sigma_overall_arcsec=0.401 sigma_q1_arcsec=0.390 sigma_q2_arcsec=0.419 sigma_q3_arcsec=0.413 sigma_q4_arcsec=0.390 n_q1=1375 n_q2=926 n_q3=1338 n_q4=868 worst_quadrant_to_overall_ratio=1.044
The image catalog is written to wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits -region wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.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.btVMTNe6M0 (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_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.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_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits
WCS-calibrated image found: wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits
Checking if the catalog wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits.wcscat corresponding to the image wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits.wcscat corresponding to the image wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits
WCS catalog name: wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.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=22, blended=2127, bad_region=8215, passed=46175
Got 46175 stars (including 36151 good ones) from the SExtractor catalog wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits.wcscat
util/solve_plate_with_UCAC5 got 46175 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4621 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4606 matched stars entering correct_measured_positions(), 4606 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4606 matched stars entering correct_measured_positions(), 39879 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4622 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4607 matched stars entering correct_measured_positions(), 39879 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 4607 matched stars entering correct_measured_positions(), 39879 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4607 stars left (next iteration limit 5066)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4607 robust_rms=6.361 arcsec worst_quadrant_rms=10.805 arcsec
SIP_REFIT: SIP order 3 trial: matched=4607 robust_rms=0.577 arcsec worst_quadrant_rms=0.703 arcsec
SIP_REFIT: SIP order 5 trial: matched=4607 robust_rms=0.403 arcsec worst_quadrant_rms=0.451 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4607 robust_rms_before=0.877 arcsec robust_rms_before_corrected=0.420 arcsec robust_rms_after=0.403 arcsec worst_quadrant_rms_before=0.476 worst_quadrant_rms_after=0.451
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.476 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits N_match=4607 sigma_overall_arcsec=0.435 sigma_q1_arcsec=0.350 sigma_q2_arcsec=0.440 sigma_q3_arcsec=0.513 sigma_q4_arcsec=0.447 n_q1=1569 n_q2=735 n_q3=1482 n_q4=821 worst_quadrant_to_overall_ratio=1.180
The image catalog is written to wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits -region wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.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.5yRlPA3CA4 (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_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.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_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
WCS-calibrated image found: wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
Checking if the catalog wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits.wcscat corresponding to the image wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits.wcscat corresponding to the image wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
WCS catalog name: wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.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=23, blended=2129, bad_region=8211, passed=45995
Got 45995 stars (including 35989 good ones) from the SExtractor catalog wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits.wcscat
util/solve_plate_with_UCAC5 got 45995 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4620 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4603 matched stars entering correct_measured_positions(), 4603 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4603 matched stars entering correct_measured_positions(), 39699 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4620 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4603 matched stars entering correct_measured_positions(), 39699 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 4603 matched stars entering correct_measured_positions(), 39699 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 4603 stars left (next iteration limit 5063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4603 robust_rms=6.394 arcsec worst_quadrant_rms=11.029 arcsec
SIP_REFIT: SIP order 3 trial: matched=4603 robust_rms=0.560 arcsec worst_quadrant_rms=0.698 arcsec
SIP_REFIT: SIP order 5 trial: matched=4603 robust_rms=0.391 arcsec worst_quadrant_rms=0.430 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4603 robust_rms_before=0.868 arcsec robust_rms_before_corrected=0.410 arcsec robust_rms_after=0.391 arcsec worst_quadrant_rms_before=0.458 worst_quadrant_rms_after=0.430
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.458 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits N_match=4603 sigma_overall_arcsec=0.420 sigma_q1_arcsec=0.349 sigma_q2_arcsec=0.432 sigma_q3_arcsec=0.486 sigma_q4_arcsec=0.419 n_q1=1581 n_q2=742 n_q3=1470 n_q4=810 worst_quadrant_to_overall_ratio=1.158
The image catalog is written to wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits -region wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.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-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.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_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-47-20_20.00sec_-0.00C_LIGHT_0288.fits
Saving fully-calibrated image wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.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_2026-08-18_CI_Aqr-02-Q2b1x1_015051_TTUQ2b1x1_3946175_txhfIMHK/wcs_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289.fits
Preparing the HTML report for the field Aqr-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:20:33.05 -04:59:06.3: 14.32 +/- 0.09 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:17:51.36 -04:14:51.2: 11.04 +/- 0.00 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:05:35.64 -02:53:55.4: 14.08 +/- 0.07 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:07:46.38 -05:55:06.5: 11.80 +/- 0.01 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:28:03.92 -05:56:44.4: 12.98 +/- 0.03 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:32:36.72 +00:06:56.1: 13.36 +/- 0.04 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:06:06.00 -01:16:33.5: 12.92 +/- 0.02 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:20:33.05 -04:59:06.3: 14.55 +/- 0.11 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:17:51.36 -04:14:51.2: 11.06 +/- 0.00 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:07:46.38 -05:55:06.5: 11.77 +/- 0.01 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.07
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:28:03.92 -05:56:44.4: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.05 +/- 0.00
Forced photometry filter REJECTED candidate at 22:20:33.05 -04:59:06.3: ref_mag=14.41 +/- 0.07 new_mean_mag=14.5732 delta=-0.16 (need > 0.90)
Forced photometry reference-image weighted average: 11.78 +/- 0.01
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:05:35.64 -02:53:55.4: 14.20 +/- 0.08 detection
Forced photometry filter REJECTED candidate at 22:07:46.38 -05:55:06.5: ref_mag=11.78 +/- 0.01 new_mean_mag=12.1049 delta=-0.32 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:17:51.36 -04:14:51.2: ref_mag=11.05 +/- 0.00 new_mean_mag=11.3632 delta=-0.31 (need > 0.90)
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Forced photometry filter REJECTED candidate at 22:28:03.92 -05:56:44.4: ref_mag=13.00 +/- 0.02 new_mean_mag=13.0365 delta=-0.04 (need > 0.90)
Forced photometry reference-image weighted average: 14.13 +/- 0.05
Forced photometry filter REJECTED candidate at 22:05:35.64 -02:53:55.4: ref_mag=14.13 +/- 0.05 new_mean_mag=14.3495 delta=-0.22 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:06:06.00 -01:16:33.5: 12.91 +/- 0.02 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:32:36.72 +00:06:56.1: 13.45 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Forced photometry filter REJECTED candidate at 22:06:06.00 -01:16:33.5: ref_mag=12.92 +/- 0.02 new_mean_mag=13.1583 delta=-0.24 (need > 0.90)
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Forced photometry filter REJECTED candidate at 22:32:36.72 +00:06:56.1: ref_mag=13.40 +/- 0.03 new_mean_mag=13.5251 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:27:05.83 -03:25:57.4: 13.70 +/- 0.06 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:26:18.56 -05:10:13.1: 13.72 +/- 0.06 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:31:47.94 -04:13:08.3: 13.92 +/- 0.07 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:27:05.83 -03:25:57.4: 13.66 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.04
Forced photometry filter REJECTED candidate at 22:27:05.83 -03:25:57.4: ref_mag=13.68 +/- 0.04 new_mean_mag=13.7864 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:26:18.56 -05:10:13.1: 13.62 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.04
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:31:47.94 -04:13:08.3: 13.90 +/- 0.07 detection
Forced photometry filter REJECTED candidate at 22:26:18.56 -05:10:13.1: ref_mag=13.67 +/- 0.04 new_mean_mag=13.7788 delta=-0.11 (need > 0.90)
Forced photometry reference-image weighted average: 13.91 +/- 0.05
Forced photometry filter REJECTED candidate at 22:31:47.94 -04:13:08.3: ref_mag=13.91 +/- 0.05 new_mean_mag=14.0477 delta=-0.14 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:01:27.84 -05:51:02.3: 13.97 +/- 0.07 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:05:28.03 -00:00:11.3: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:30:43.29 +00:18:59.3: 14.28 +/- 0.09 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:31:10.04 -02:25:15.9: 14.55 +/- 0.11 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:14:28.68 +02:03:47.7: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:01:27.84 -05:51:02.3: 13.95 +/- 0.07 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:28:07.39 -02:07:03.9: 14.23 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.05
Forced photometry filter REJECTED candidate at 22:01:27.84 -05:51:02.3: ref_mag=13.96 +/- 0.05 new_mean_mag=13.9713 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:03:57.67 -05:38:47.5: 15.02 +/- 0.18 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:30:43.29 +00:18:59.3: 14.51 +/- 0.11 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:05:28.03 -00:00:11.3: 15.87 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.37 +/- 0.07
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:31:10.04 -02:25:15.9: 14.71 +/- 0.13 detection
Forced photometry filter REJECTED candidate at 22:30:43.29 +00:18:59.3: ref_mag=14.37 +/- 0.07 new_mean_mag=14.4092 delta=-0.04 (need > 0.90)
Forced photometry reference-image weighted average: 14.62 +/- 0.09
Forced photometry filter REJECTED candidate at 22:31:10.04 -02:25:15.9: ref_mag=14.62 +/- 0.09 new_mean_mag=14.5737 delta=0.04 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:14:28.68 +02:03:47.7: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:28:51.60 +01:53:52.4: 14.66 +/- 0.13 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:03:57.67 -05:38:47.5: 14.74 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.84 +/- 0.11
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:00:18.13 -03:10:19.1: 15.91 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 22:03:57.67 -05:38:47.5: ref_mag=14.84 +/- 0.11 new_mean_mag=14.6371 delta=0.20 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:28:07.39 -02:07:03.9: 14.33 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.27 +/- 0.06
Forced photometry filter REJECTED candidate at 22:28:07.39 -02:07:03.9: ref_mag=14.27 +/- 0.06 new_mean_mag=14.5753 delta=-0.30 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:28:51.60 +01:53:52.4: 14.58 +/- 0.11 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:30:35.96 -00:46:56.2: 14.46 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.62 +/- 0.08
Forced photometry filter REJECTED candidate at 22:28:51.60 +01:53:52.4: ref_mag=14.62 +/- 0.08 new_mean_mag=14.4205 delta=0.19 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:00:18.13 -03:10:19.1: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:05:13.73 -05:06:40.3: 15.39 +/- 0.26 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:30:35.96 -00:46:56.2: 14.50 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.48 +/- 0.07
Forced photometry filter REJECTED candidate at 22:30:35.96 -00:46:56.2: ref_mag=14.48 +/- 0.07 new_mean_mag=14.4606 delta=0.02 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:29:07.88 -05:52:16.6: 15.19 +/- 0.23 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:02:10.75 -05:36:47.1: 15.39 +/- 0.26 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:05:13.73 -05:06:40.3: 14.96 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.08 +/- 0.14
Forced photometry filter REJECTED candidate at 22:05:13.73 -05:06:40.3: ref_mag=15.08 +/- 0.14 new_mean_mag=14.6864 delta=0.39 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:01:03.97 -06:11:48.8: 15.31 +/- 0.24 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:09:27.01 -03:02:46.1: 15.16 +/- 0.18 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:12:09.49 -03:52:30.6: 14.63 +/- 0.11 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:29:07.88 -05:52:16.6: 15.50 +/- 0.30 detection
Forced photometry reference-image weighted average: 15.31 +/- 0.18
Forced photometry filter REJECTED candidate at 22:29:07.88 -05:52:16.6: ref_mag=15.31 +/- 0.18 new_mean_mag=14.7806 delta=0.53 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:02:10.75 -05:36:47.1: 15.02 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.14 +/- 0.15
Forced photometry filter REJECTED candidate at 22:02:10.75 -05:36:47.1: ref_mag=15.14 +/- 0.15 new_mean_mag=14.8475 delta=0.29 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:01:03.97 -06:11:48.8: 15.35 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.33 +/- 0.17
Forced photometry filter REJECTED candidate at 22:01:03.97 -06:11:48.8: ref_mag=15.33 +/- 0.17 new_mean_mag=14.7604 delta=0.57 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:09:27.01 -03:02:46.1: 14.94 +/- 0.15 detection
Forced photometry reference-image weighted average: 15.03 +/- 0.11
Forced photometry filter REJECTED candidate at 22:09:27.01 -03:02:46.1: ref_mag=15.03 +/- 0.11 new_mean_mag=14.7433 delta=0.28 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:12:09.49 -03:52:30.6: 14.78 +/- 0.13 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:25:49.14 -05:22:15.2: 14.93 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.69 +/- 0.08
Forced photometry filter REJECTED candidate at 22:12:09.49 -03:52:30.6: ref_mag=14.69 +/- 0.08 new_mean_mag=14.6128 delta=0.08 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:12:59.18 -04:02:37.7: 14.96 +/- 0.16 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:25:49.14 -05:22:15.2: 14.79 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.84 +/- 0.11
Forced photometry filter REJECTED candidate at 22:25:49.14 -05:22:15.2: ref_mag=14.84 +/- 0.11 new_mean_mag=14.6567 delta=0.19 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:07:50.67 -04:27:00.1: 15.54 +/- 0.27 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:07:56.65 -05:27:52.7: 14.75 +/- 0.15 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:12:59.18 -04:02:37.7: 15.17 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.04 +/- 0.12
Forced photometry filter REJECTED candidate at 22:12:59.18 -04:02:37.7: ref_mag=15.04 +/- 0.12 new_mean_mag=14.7427 delta=0.30 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:34:10.55 +00:50:15.4: 15.09 +/- 0.19 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:30:13.27 +02:15:09.5: 15.21 +/- 0.20 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:00:08.88 -02:53:37.1: 15.12 +/- 0.19 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:07:50.67 -04:27:00.1: 15.47 +/- 0.26 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:07:56.65 -05:27:52.7: 15.06 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.50 +/- 0.19
Forced photometry filter REJECTED candidate at 22:07:50.67 -04:27:00.1: ref_mag=15.50 +/- 0.19 new_mean_mag=14.8509 delta=0.65 (need > 0.90)
Forced photometry reference-image weighted average: 14.86 +/- 0.12
Forced photometry filter REJECTED candidate at 22:07:56.65 -05:27:52.7: ref_mag=14.86 +/- 0.12 new_mean_mag=14.8137 delta=0.04 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:34:10.55 +00:50:15.4: 15.16 +/- 0.20 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:30:13.27 +02:15:09.5: 14.96 +/- 0.16 detection
Forced photometry reference-image weighted average: 15.12 +/- 0.14
Forced photometry filter REJECTED candidate at 22:34:10.55 +00:50:15.4: ref_mag=15.12 +/- 0.14 new_mean_mag=14.8264 delta=0.29 (need > 0.90)
Forced photometry reference-image weighted average: 15.05 +/- 0.13
Forced photometry filter REJECTED candidate at 22:30:13.27 +02:15:09.5: ref_mag=15.05 +/- 0.13 new_mean_mag=14.8146 delta=0.24 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:00:08.88 -02:53:37.1: 14.88 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.97 +/- 0.11
Forced photometry filter REJECTED candidate at 22:00:08.88 -02:53:37.1: ref_mag=14.97 +/- 0.11 new_mean_mag=14.7585 delta=0.21 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:14:07.92 -04:41:15.4: 14.64 +/- 0.13 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:14:07.92 -04:41:15.4: 14.81 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.71 +/- 0.09
Forced photometry filter KEPT candidate at 22:14:07.92 -04:41:15.4: ref_mag=14.71 +/- 0.09 new_mean_mag=13.6243 delta=1.09 (need > 0.90)
Adding exclusion_list_local.txt__out41053.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61531.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 12s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
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Considering the candidate 53086_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 53086_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 53090_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 53090_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 53091_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 53091_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 53098_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 53098_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 53101_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 53101_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 53103_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 53103_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 53105_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 53105_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 54300_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 54300_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
**** FOUND 22:33:54.56 -01:34:14.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 55834_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 55834_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 57290_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 57290_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 57833_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 57833_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 58146_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 58146_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 58760_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 58760_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 58775_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 58775_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 59908_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
Preparing report for the candidate 59908_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
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Considering the candidate 60843_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 60843_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 60925_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 60925_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 60951_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
Preparing report for the candidate 60951_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
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Considering the candidate 60999_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 60999_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 61241_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 61241_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 61382_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 61382_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 61405_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 61405_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 61531_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
Preparing report for the candidate 61531_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
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Considering the candidate 61866_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 61866_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 61965_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 61965_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 62115_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 62115_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 62124_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 62124_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 62232_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 62232_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 62241_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 62241_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 62380_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 62380_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 62402_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 62402_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 62596_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 62596_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 62644_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 62644_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 62709_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 62709_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 62835_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 62835_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 62892_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289
The candidate 62892_fd_Aqr-02-Q2b1x1_2026-08-18_01-48-13_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks