This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA
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 05 31.3742 2461191.8742 11.18 22:41:01.22 -14:22:47.5
49.07335 -57.08633 galactic Aqr Second-epoch detections are separated by 1.4" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.9 Metis -1 -1 1 11.1 -0 -0
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:41:01.22 -14:22:47.5: 14.73 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:41:01.22 -14:22:47.5: 14.74 +/- 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,2461191.8742,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260531.3742 11.18CV 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 05 31.3742 2461191.8742 12.37 22:11:14.34 -11:17:55.8
47.83371 -49.23629 galactic Aqr Second-epoch detections are separated by 0.5" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.100 Hekate -1 -1 1 12.6 0 0
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:11:14.34 -11:17:55.8: 15.16 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:11:14.34 -11:17:55.8: 15.17 +/- 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,2461191.8742,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260531.3742 12.37CV 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 05 31.3742 2461191.8742 12.54 22:45:07.47 -07:48:49.3
59.88967 -54.40538 galactic Aqr Second-epoch detections are separated by 1.3" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.5 Astraea -1 -2 2 12.7 0 0
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:45:07.47 -07:48:49.3: 14.84 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:45:07.47 -07:48:49.3: 14.84 +/- 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,2461191.8742,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260531.3742 12.54CV 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 05 31.3742 2461191.8742 13.32 22:05:27.98 -06:50:56.1
52.43504 -45.74611 galactic Aqr Second-epoch detections are separated by 1.8" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.476 Hedwig -1 -1 1 13.4 0 0
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:05:27.98 -06:50:56.1: 15.14 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:05:27.98 -06:50:56.1: 15.14 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461191.8742,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260531.3742 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461177.89902836 17.05.2026 09:34:26.050 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
First image: 2461177.89902836 17.05.2026 09:34:26.050 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
Last image: 2461191.87450098 31.05.2026 08:59:06.885 /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.07
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 4307
Objects passed selection criteria: 4305
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 3891
Average stars matched: 3837.25 (98.6186 %)
Memory usage VmPeak: 110512 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue May 26 15:05:11 CDT 2026
VaST build number 1.0rc89-83-g49118af2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-26)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun May 31 04:21:32 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461177.89902836 17.05.2026 09:34:26.050 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
First image: 2461177.89902836 17.05.2026 09:34:26.050 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
Last image: 2461191.87450098 31.05.2026 08:59:06.885 /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.85
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: 16 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 25093
Objects passed selection criteria: 25058
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 21526.8
Average stars matched: 20931.2 (97.2337 %)
Memory usage VmPeak: 129320 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue May 26 15:05:11 CDT 2026
VaST build number 1.0rc89-83-g49118af2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-26)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun May 31 04:24:04 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
SExtractor catalog cache: saved Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat to cache
SExtractor catalog cache: saved Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.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: 2461191.87390179
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits exists and is non-empty
Saving wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits to local_wcs_cache/
'wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits' -> 'local_wcs_cache/wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits'
wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits exists and is non-empty
Saving wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits to local_wcs_cache/
'wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits' -> 'local_wcs_cache/wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits'
wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits exists and is non-empty
Saving wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits to local_wcs_cache/
'wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits' -> 'local_wcs_cache/wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits'
wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits exists and is non-empty
Saving wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits to local_wcs_cache/
'wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits' -> 'local_wcs_cache/wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits (1st reference image)
verification OK: wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
Image size: 942.7'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:17:06.962 -09:59:19.64 J2000 4789.000 3195.000
###################################
The image scale is 5.91"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits (1st new image)
verification OK: wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits
Image size: 941.9'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:17:15.845 -10:02:21.35 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:17:06.962 -09:59:19.64
Second-epoch image center 22:17:15.845 -10:02:21.35
Angular distance between the image centers 0.0623 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits (2nd new image)
verification OK: wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
Image size: 941.9'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:17:18.989 -10:01:49.20 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:17:06.962 -09:59:19.64
Second-epoch image center 22:17:18.989 -10:01:49.20
Angular distance between the image centers 0.0645 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 22:17:15.845 -10:02:21.35
Second-epoch second image center 22:17:18.989 -10:01:49.20
Angular distance between the image centers 0.01569 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits &> /tmp/tmp.vLnBbpE98X
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits &> /tmp/tmp.7QaRIL3I9x
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits &> /tmp/tmp.7FjTSOU7I1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits &> /tmp/tmp.MkOEA1ltu1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits and wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits and wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat
Found non-empty wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits and wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat
The reference image (wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits) and catalog (wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat) found
'wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat' -> 'wcsmag.cat'
Read 4529 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.9175 to 342.3809 deg, Dec -15.5885 to -4.2887 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 325.9175 to 342.3809 deg, Dec -15.5885 to -4.2887 deg
Loaded 5486 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): 3405 out of 3455 total matches.
Matched with Tycho-2 3455 out of 4529 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.448200
a=0.000000 b=1.000000 c=22.448200
From vast_summary.log: estimated ref. image limiting mag.: -8.07
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.38
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.38
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 4529 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.9175 to 342.3809 deg, Dec -15.5885 to -4.2887 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 325.9175 to 342.3809 deg, Dec -15.5885 to -4.2887 deg
Loaded 5486 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): 3405 out of 3455 total matches.
Matched with Tycho-2 3455 out of 4529 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits -> calib.txt_param_ref_wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits (aperture=6.2)
Read 4507 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.9176 to 342.3811 deg, Dec -15.5918 to -4.2887 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 325.9176 to 342.3811 deg, Dec -15.5918 to -4.2887 deg
Loaded 5486 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): 3392 out of 3444 total matches.
Matched with Tycho-2 3444 out of 4507 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits -> calib.txt_param_ref_wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.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: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
2.4 pix Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
3.7 pix fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits
3.7 pix fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
2.4 pix wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
2.4 pix wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
Limiting magnitude estimates:
14.4 mag. Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
14.4 mag. Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
13.7 mag. fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits
13.8 mag. fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 11.2 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.vLnBbpE98X (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_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits' -> 'wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
WCS-calibrated image found: wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
Checking if the catalog wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
WCS catalog name: wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=254, passed=4529
Got 4529 stars (including 4272 good ones) from the SExtractor catalog wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat
util/solve_plate_with_UCAC5 got 4529 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010474 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 886 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 883 matched stars entering correct_measured_positions(), 873 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 883 matched stars entering correct_measured_positions(), 4460 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 885 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 883 matched stars entering correct_measured_positions(), 4460 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 883 matched stars entering correct_measured_positions(), 4460 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 883 stars left (next iteration limit 971)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits N_match=883 sigma_overall_arcsec=0.292 sigma_q1_arcsec=0.300 sigma_q2_arcsec=0.317 sigma_q3_arcsec=0.250 sigma_q4_arcsec=0.318 n_q1=255 n_q2=171 n_q3=261 n_q4=196 worst_quadrant_to_overall_ratio=1.091
The image catalog is written to wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits -region wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.7QaRIL3I9x (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_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits' -> 'wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
WCS-calibrated image found: wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
Checking if the catalog wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.cat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.cat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
WCS catalog name: wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=252, passed=4507
Got 4507 stars (including 4252 good ones) from the SExtractor catalog wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.cat
util/solve_plate_with_UCAC5 got 4507 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010474 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 881 matched stars entering correct_measured_positions(), 868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 881 matched stars entering correct_measured_positions(), 4429 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 883 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 881 matched stars entering correct_measured_positions(), 4427 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 881 matched stars entering correct_measured_positions(), 4427 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 881 stars left (next iteration limit 969)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits N_match=881 sigma_overall_arcsec=0.285 sigma_q1_arcsec=0.282 sigma_q2_arcsec=0.347 sigma_q3_arcsec=0.234 sigma_q4_arcsec=0.302 n_q1=256 n_q2=169 n_q3=258 n_q4=198 worst_quadrant_to_overall_ratio=1.218
The image catalog is written to wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits -region wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.7FjTSOU7I1 (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_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.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_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits
Checking if the catalog wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits.cat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits.cat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits
WCS catalog name: wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=200, passed=3287
Got 3287 stars (including 3087 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits.cat
util/solve_plate_with_UCAC5 got 3287 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.4)
Done reading UCAC5 zone files...
Matched 879 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 876 matched stars entering correct_measured_positions(), 863 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 876 matched stars entering correct_measured_positions(), 3234 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.4)
Done reading UCAC5 zone files...
Matched 878 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 876 matched stars entering correct_measured_positions(), 3235 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 876 matched stars entering correct_measured_positions(), 3235 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 876 stars left (next iteration limit 963)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits N_match=876 sigma_overall_arcsec=0.273 sigma_q1_arcsec=0.297 sigma_q2_arcsec=0.302 sigma_q3_arcsec=0.207 sigma_q4_arcsec=0.269 n_q1=249 n_q2=174 n_q3=254 n_q4=199 worst_quadrant_to_overall_ratio=1.108
The image catalog is written to wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits -region wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.MkOEA1ltu1 (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_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.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_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
Checking if the catalog wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits.cat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits.cat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
WCS catalog name: wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=207, passed=3322
Got 3322 stars (including 3110 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits.cat
util/solve_plate_with_UCAC5 got 3322 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.4)
Done reading UCAC5 zone files...
Matched 880 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 877 matched stars entering correct_measured_positions(), 864 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 877 matched stars entering correct_measured_positions(), 3260 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.4)
Done reading UCAC5 zone files...
Matched 879 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 877 matched stars entering correct_measured_positions(), 3260 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 877 matched stars entering correct_measured_positions(), 3260 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 877 stars left (next iteration limit 964)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits N_match=877 sigma_overall_arcsec=0.265 sigma_q1_arcsec=0.269 sigma_q2_arcsec=0.306 sigma_q3_arcsec=0.232 sigma_q4_arcsec=0.261 n_q1=251 n_q2=169 n_q3=258 n_q4=199 worst_quadrant_to_overall_ratio=1.155
The image catalog is written to wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits -region wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits sigma_overall=0.292 worst_q_ratio=1.091
ref2=Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits sigma_overall=0.285 worst_q_ratio=1.218
new1=fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits sigma_overall=0.273 worst_q_ratio=1.108
new2=fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits sigma_overall=0.265 worst_q_ratio=1.155
reference average sigma_overall=0.2885 worst_q_ratio=1.1545
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446_astrometric_residuals.png (883 matched stars from wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447_astrometric_residuals.png (881 matched stars from wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370_astrometric_residuals.png (876 matched stars from wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371_astrometric_residuals.png (877 matched stars from wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits'
Saving fully-calibrated image wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits'
Preparing the HTML report for the field Aqr-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:41:01.22 -14:22:47.5: 14.73 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:41:01.22 -14:22:47.5: 14.74 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out20213.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20213_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371
Preparing report for the candidate 20213_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 9s
Prepared the HTML report for the field Aqr-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
22:41:01.22 -14:22:47.5
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
SExtractor catalog cache: saved Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat to cache
SExtractor catalog cache: saved Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
Creating symlink local_wcs_cache/wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits exists and is non-empty
wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits exists and is non-empty
wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits exists and is non-empty
wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits (1st reference image)
verification OK: wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
Image size: 942.7'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:17:06.962 -09:59:19.64 J2000 4789.000 3195.000
###################################
The image scale is 5.91"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits (1st new image)
verification OK: wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits
Image size: 941.9'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:17:15.845 -10:02:21.35 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:17:06.962 -09:59:19.64
Second-epoch image center 22:17:15.845 -10:02:21.35
Angular distance between the image centers 0.0623 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits (2nd new image)
verification OK: wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
Image size: 941.9'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:17:18.989 -10:01:49.20 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:17:06.962 -09:59:19.64
Second-epoch image center 22:17:18.989 -10:01:49.20
Angular distance between the image centers 0.0645 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 22:17:15.845 -10:02:21.35
Second-epoch second image center 22:17:18.989 -10:01:49.20
Angular distance between the image centers 0.01569 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits &> /tmp/tmp.RWDORNsDNK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits &> /tmp/tmp.Lkt3FgJIBd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits &> /tmp/tmp.eybKPpy0mJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits &> /tmp/tmp.DkT4TNL1TS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits and wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits and wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat
Found non-empty wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits and wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat
The reference image (wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits) and catalog (wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat) found
'wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat' -> 'wcsmag.cat'
Read 27177 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.8701 to 342.4551 deg, Dec -15.5885 to -4.2463 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 325.8701 to 342.4551 deg, Dec -15.5885 to -4.2463 deg
Loaded 5550 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): 4272 out of 4485 total matches.
Matched with Tycho-2 4485 out of 27177 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.318600
a=0.000000 b=1.000000 c=22.318600
From vast_summary.log: estimated ref. image limiting mag.: -7.85
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.47
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 27177 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.8701 to 342.4551 deg, Dec -15.5885 to -4.2463 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 325.8701 to 342.4551 deg, Dec -15.5885 to -4.2463 deg
Loaded 5550 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): 4272 out of 4485 total matches.
Matched with Tycho-2 4485 out of 27177 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits -> calib.txt_param_ref_wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits (aperture=5.1)
Read 27357 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.8701 to 342.4399 deg, Dec -15.6108 to -4.2411 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 325.8701 to 342.4399 deg, Dec -15.6108 to -4.2411 deg
Loaded 5555 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): 4272 out of 4487 total matches.
Matched with Tycho-2 4487 out of 27357 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits -> calib.txt_param_ref_wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits (aperture=5.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
2.4 pix Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
3.5 pix fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits
3.4 pix fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
2.4 pix wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
2.4 pix wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
Limiting magnitude estimates:
14.5 mag. Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
14.5 mag. Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
13.8 mag. fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits
13.8 mag. fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 13.1 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.RWDORNsDNK (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_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits' -> 'wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
WCS-calibrated image found: wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
Checking if the catalog wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
WCS catalog name: wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=866, passed=27172
Got 27172 stars (including 26255 good ones) from the SExtractor catalog wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat
util/solve_plate_with_UCAC5 got 27172 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010474 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 882 matched stars entering correct_measured_positions(), 867 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 882 matched stars entering correct_measured_positions(), 26772 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 883 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 882 matched stars entering correct_measured_positions(), 26771 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 882 matched stars entering correct_measured_positions(), 26771 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 882 stars left (next iteration limit 970)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits N_match=882 sigma_overall_arcsec=0.293 sigma_q1_arcsec=0.285 sigma_q2_arcsec=0.325 sigma_q3_arcsec=0.253 sigma_q4_arcsec=0.339 n_q1=253 n_q2=170 n_q3=268 n_q4=191 worst_quadrant_to_overall_ratio=1.157
The image catalog is written to wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits -region wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Lkt3FgJIBd (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_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits' -> 'wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
WCS-calibrated image found: wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
Checking if the catalog wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.cat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.cat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
WCS catalog name: wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=827, passed=27349
Got 27349 stars (including 26484 good ones) from the SExtractor catalog wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.cat
util/solve_plate_with_UCAC5 got 27349 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010474 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 882 matched stars entering correct_measured_positions(), 863 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 882 matched stars entering correct_measured_positions(), 26905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 883 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 882 matched stars entering correct_measured_positions(), 26909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 882 matched stars entering correct_measured_positions(), 26909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 882 stars left (next iteration limit 970)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits N_match=882 sigma_overall_arcsec=0.286 sigma_q1_arcsec=0.265 sigma_q2_arcsec=0.384 sigma_q3_arcsec=0.248 sigma_q4_arcsec=0.303 n_q1=254 n_q2=169 n_q3=267 n_q4=192 worst_quadrant_to_overall_ratio=1.342
The image catalog is written to wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits -region wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.eybKPpy0mJ (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_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.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_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits
Checking if the catalog wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits.cat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits.cat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits
WCS catalog name: wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=515, passed=15902
Got 15902 stars (including 15367 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits.cat
util/solve_plate_with_UCAC5 got 15902 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 879 matched stars entering correct_measured_positions(), 865 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 879 matched stars entering correct_measured_positions(), 15692 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 880 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 879 matched stars entering correct_measured_positions(), 15693 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 879 matched stars entering correct_measured_positions(), 15693 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 879 stars left (next iteration limit 966)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits N_match=879 sigma_overall_arcsec=0.292 sigma_q1_arcsec=0.311 sigma_q2_arcsec=0.318 sigma_q3_arcsec=0.234 sigma_q4_arcsec=0.285 n_q1=242 n_q2=166 n_q3=267 n_q4=204 worst_quadrant_to_overall_ratio=1.088
The image catalog is written to wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits -region wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.DkT4TNL1TS (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_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.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_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
Checking if the catalog wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits.cat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits.cat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
WCS catalog name: wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=570, passed=16285
Got 16285 stars (including 15698 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits.cat
util/solve_plate_with_UCAC5 got 16285 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 880 matched stars entering correct_measured_positions(), 866 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 880 matched stars entering correct_measured_positions(), 16049 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 880 matched stars entering correct_measured_positions(), 16048 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 880 matched stars entering correct_measured_positions(), 16048 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 880 stars left (next iteration limit 968)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits N_match=880 sigma_overall_arcsec=0.272 sigma_q1_arcsec=0.260 sigma_q2_arcsec=0.308 sigma_q3_arcsec=0.237 sigma_q4_arcsec=0.298 n_q1=247 n_q2=163 n_q3=266 n_q4=204 worst_quadrant_to_overall_ratio=1.129
The image catalog is written to wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits -region wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.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_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-58-15_20.00sec_0.00C_LIGHTs_0370.fits
Saving fully-calibrated image wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.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_2026-05-31_CI_Aqr-04-Q1b1x1_041347_TTUQ1b1x1_1233930_TGZgT4vA/wcs_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371.fits
Preparing the HTML report for the field Aqr-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:26:06.88 -05:09:40.8: 12.83 +/- 0.05 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:45:07.47 -07:48:49.3: 14.84 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:11:14.34 -11:17:55.8: 15.16 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:05:27.98 -06:50:56.1: 15.14 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:26:02.95 -05:10:21.7: 12.71 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:11:14.34 -11:17:55.8: 15.17 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:26:06.88 -05:09:40.8: 12.81 +/- 0.05 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:45:07.47 -07:48:49.3: 14.84 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.82 +/- 0.04
Forced photometry filter REJECTED candidate at 22:26:06.88 -05:09:40.8: ref_mag=12.82 +/- 0.04 new_mean_mag=12.7773 delta=0.04 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:05:27.98 -06:50:56.1: 15.14 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:26:02.95 -05:10:21.7: 12.82 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.03
Forced photometry filter REJECTED candidate at 22:26:02.95 -05:10:21.7: ref_mag=12.76 +/- 0.03 new_mean_mag=12.7649 delta=-0.01 (need > 0.90)
Adding exclusion_list_local.txt__out32212.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32218.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32246.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32187_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371
The candidate 32187_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371 did not pass the final checks
**** FOUND 22:41:01.23 -14:22:47.7 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32212_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371
Preparing report for the candidate 32212_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32218_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371
Preparing report for the candidate 32218_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32222_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371
The candidate 32222_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32225_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371
The candidate 32225_fd_Aqr-04-Q1b1x1_2026-05-31_03-59-06_20.00sec_-0.00C_LIGHTs_0371 did not pass the final checks