This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 08 06.2769 2461258.7769 10.71 21:26:38.61 -13:38:04.3
38.05369 -40.50081 galactic Aqr Second-epoch detections are separated by 0.4" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.306 Unitas -0 0 0 10.6 0 -0
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:26:38.61 -13:38:04.3: 15.44 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:26:38.61 -13:38:04.3: 15.47 +/- 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,2461258.7769,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260806.2769 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2769 2461258.7769 11.46 21:21:52.30 -07:26:13.9
44.49565 -36.69669 galactic Aqr Second-epoch detections are separated by 0.3" 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.389 Industria -0 0 1 11.6 0 0
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:21:52.30 -07:26:13.9: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:21:52.30 -07:26:13.9: 15.67 +/- 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,2461258.7769,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260806.2769 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2769 2461258.7769 12.46 21:19:12.54 -11:39:09.6
39.39310 -38.02262 galactic Aqr Second-epoch detections are separated by 0.5" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.38 Leda -0 0 0 12.8 -0 -0
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:19:12.54 -11:39:09.6: 15.60 +/- 0.34 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:19:12.54 -11:39:09.6: 15.66 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.60 +/- 0.34
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,2461258.7769,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260806.2769 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2769 2461258.7769 13.18 21:20:00.72 -13:55:00.6
36.86478 -39.14481 galactic Aqr Second-epoch detections are separated by 1.6" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.558 Carmen 0 -0 0 13.1 0 -0
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:20:00.72 -13:55:00.6: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:20:00.72 -13:55:00.6: 15.60 +/- 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,2461258.7769,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260806.2769 13.18CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461209.88890352 18.06.2026 09:19:51.264 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
First image: 2461209.88890352 18.06.2026 09:19:51.264 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
Last image: 2461258.77721101 06.08.2026 06:39:01.031 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.82
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 5945
Objects passed selection criteria: 5937
Measurements per detected object (mean, median, min, max): 2.9 3.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 3.0 2 4
Average stars detected per image: 5186
Average stars matched: 4644.25 (89.5536 %)
Memory usage VmPeak: 233480 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Aug 5 15:05:04 CDT 2026
VaST build number 1.0rc89-189-g49d3cdfd
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-05)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Aug 6 02:19:37 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: 2461209.88890352 18.06.2026 09:19:51.264 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
First image: 2461209.88890352 18.06.2026 09:19:51.264 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
Last image: 2461258.77721101 06.08.2026 06:39:01.031 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 26
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.52
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 11 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 38732
Objects passed selection criteria: 38674
Measurements per detected object (mean, median, min, max): 3.2 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 3.0 2 4
Average stars detected per image: 35213
Average stars matched: 32172.8 (91.3661 %)
Memory usage VmPeak: 265440 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Aug 5 15:05:04 CDT 2026
VaST build number 1.0rc89-189-g49d3cdfd
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-05)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Aug 6 02:20:31 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
SExtractor catalog cache: saved Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.cat to cache
SExtractor catalog cache: saved Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.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: 2461258.77657509
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits exists and is non-empty
Saving wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits to local_wcs_cache/
'wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits' -> 'local_wcs_cache/wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits'
wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits exists and is non-empty
Saving wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits to local_wcs_cache/
'wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits' -> 'local_wcs_cache/wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits'
wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits exists and is non-empty
Saving wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits to local_wcs_cache/
'wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits' -> 'local_wcs_cache/wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits'
wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits exists and is non-empty
Saving wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits to local_wcs_cache/
'wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits' -> 'local_wcs_cache/wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits (1st reference image)
verification OK: wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
Image size: 937.4'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:25:43.484 -09:59:39.66 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits (1st new image)
verification OK: wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
Image size: 937.0'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:25:43.371 -09:59:43.71 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:25:43.484 -09:59:39.66
Second-epoch image center 21:25:43.371 -09:59:43.71
Angular distance between the image centers 0.0012 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits (2nd new image)
verification OK: wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
Image size: 937.0'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:25:40.380 -10:00:13.34 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:25:43.484 -09:59:39.66
Second-epoch image center 21:25:40.380 -10:00:13.34
Angular distance between the image centers 0.0158 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 21:25:43.371 -09:59:43.71
Second-epoch second image center 21:25:40.380 -10:00:13.34
Angular distance between the image centers 0.01478 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits &> /tmp/tmp.lIwKKXNzqg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits &> /tmp/tmp.VRpW43DbH3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits &> /tmp/tmp.M9QHt5c53u
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits &> /tmp/tmp.NV54BJUbRL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits and wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits and wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat
Found non-empty wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits and wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat
The reference image (wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits) and catalog (wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat) found
'wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat' -> 'wcsmag.cat'
Read 8874 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.3905 to 329.4911 deg, Dec -15.2504 to -4.7005 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 313.3905 to 329.4911 deg, Dec -15.2504 to -4.7005 deg
Loaded 6721 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): 5451 out of 5615 total matches.
Matched with Tycho-2 5615 out of 8874 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.686800
a=0.000000 b=1.000000 c=22.686800
From vast_summary.log: estimated ref. image limiting mag.: -7.82
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.87
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.87
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 8874 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.3905 to 329.4911 deg, Dec -15.2504 to -4.7005 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 313.3905 to 329.4911 deg, Dec -15.2504 to -4.7005 deg
Loaded 6721 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): 5451 out of 5615 total matches.
Matched with Tycho-2 5615 out of 8874 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
Forced-photometry filter: calibrated wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits -> calib.txt_param_ref_wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits (aperture=6.3)
Read 9225 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.3619 to 329.4904 deg, Dec -15.2503 to -4.7004 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 313.3619 to 329.4904 deg, Dec -15.2503 to -4.7004 deg
Loaded 6736 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): 5526 out of 5688 total matches.
Matched with Tycho-2 5688 out of 9225 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
Forced-photometry filter: calibrated wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits -> calib.txt_param_ref_wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
2.4 pix Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
2.2 pix fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
2.2 pix fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
Limiting magnitude estimates:
14.9 mag. Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
14.9 mag. Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
14.1 mag. fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
14.0 mag. fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.lIwKKXNzqg (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits' -> 'wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
WCS_IMAGE_NAME=wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
WCS-calibrated image found: wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
Checking if the catalog wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat corresponding to the image wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits alredy exist and is non-empty...
Catalog wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat corresponding to the image wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
WCS catalog name: wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=515, bad_region=1806, passed=8874
Got 8874 stars (including 6632 good ones) from the SExtractor catalog wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat
util/solve_plate_with_UCAC5 got 8874 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4800 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4772 matched stars entering correct_measured_positions(), 4772 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4772 matched stars entering correct_measured_positions(), 7430 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4800 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4771 matched stars entering correct_measured_positions(), 7430 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4771 matched stars entering correct_measured_positions(), 7430 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4771 stars left (next iteration limit 5249)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits N_match=4771 sigma_overall_arcsec=0.327 sigma_q1_arcsec=0.313 sigma_q2_arcsec=0.311 sigma_q3_arcsec=0.357 sigma_q4_arcsec=0.300 n_q1=1633 n_q2=774 n_q3=1589 n_q4=775 worst_quadrant_to_overall_ratio=1.093
The image catalog is written to wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits -region wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.VRpW43DbH3 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits' -> 'wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
WCS_IMAGE_NAME=wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
WCS-calibrated image found: wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
Checking if the catalog wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat corresponding to the image wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits alredy exist and is non-empty...
Catalog wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat corresponding to the image wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
WCS catalog name: wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=511, bad_region=2466, passed=9225
Got 9225 stars (including 6353 good ones) from the SExtractor catalog wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat
util/solve_plate_with_UCAC5 got 9225 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4685 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4657 matched stars entering correct_measured_positions(), 4657 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4657 matched stars entering correct_measured_positions(), 7282 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4686 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4658 matched stars entering correct_measured_positions(), 7282 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4658 matched stars entering correct_measured_positions(), 7282 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4658 stars left (next iteration limit 5122)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits N_match=4658 sigma_overall_arcsec=0.360 sigma_q1_arcsec=0.317 sigma_q2_arcsec=0.404 sigma_q3_arcsec=0.352 sigma_q4_arcsec=0.385 n_q1=1453 n_q2=888 n_q3=1350 n_q4=967 worst_quadrant_to_overall_ratio=1.121
The image catalog is written to wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits -region wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.M9QHt5c53u (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
WCS-calibrated image found: wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
Checking if the catalog wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
WCS catalog name: wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=294, bad_region=891, passed=4478
Got 4478 stars (including 3339 good ones) from the SExtractor catalog wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits.wcscat
util/solve_plate_with_UCAC5 got 4478 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 3209 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3196 matched stars entering correct_measured_positions(), 3196 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3196 matched stars entering correct_measured_positions(), 3733 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 3209 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3196 matched stars entering correct_measured_positions(), 3733 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 3196 matched stars entering correct_measured_positions(), 3733 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 3196 stars left (next iteration limit 3515)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3196 robust_rms=7.125 arcsec worst_quadrant_rms=10.733 arcsec
SIP_REFIT: SIP order 3 trial: matched=3196 robust_rms=0.446 arcsec worst_quadrant_rms=0.526 arcsec
SIP_REFIT: SIP order 5 trial: matched=3196 robust_rms=0.373 arcsec worst_quadrant_rms=0.388 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3196 robust_rms_before=0.850 arcsec robust_rms_before_corrected=0.401 arcsec robust_rms_after=0.373 arcsec worst_quadrant_rms_before=0.419 worst_quadrant_rms_after=0.388
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.419 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits N_match=3196 sigma_overall_arcsec=0.414 sigma_q1_arcsec=0.378 sigma_q2_arcsec=0.448 sigma_q3_arcsec=0.435 sigma_q4_arcsec=0.407 n_q1=1213 n_q2=489 n_q3=1051 n_q4=443 worst_quadrant_to_overall_ratio=1.081
The image catalog is written to wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits -region wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.NV54BJUbRL (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
WCS-calibrated image found: wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
Checking if the catalog wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
WCS catalog name: wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=292, bad_region=797, passed=4242
Got 4242 stars (including 3198 good ones) from the SExtractor catalog wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits.wcscat
util/solve_plate_with_UCAC5 got 4242 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 3075 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3061 matched stars entering correct_measured_positions(), 3061 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3061 matched stars entering correct_measured_positions(), 3573 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 3076 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3061 matched stars entering correct_measured_positions(), 3573 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 3061 matched stars entering correct_measured_positions(), 3573 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 3061 stars left (next iteration limit 3367)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3061 robust_rms=6.965 arcsec worst_quadrant_rms=11.116 arcsec
SIP_REFIT: SIP order 3 trial: matched=3061 robust_rms=0.448 arcsec worst_quadrant_rms=0.550 arcsec
SIP_REFIT: SIP order 5 trial: matched=3061 robust_rms=0.366 arcsec worst_quadrant_rms=0.402 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3061 robust_rms_before=0.806 arcsec robust_rms_before_corrected=0.396 arcsec robust_rms_after=0.366 arcsec worst_quadrant_rms_before=0.428 worst_quadrant_rms_after=0.402
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.428 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits N_match=3061 sigma_overall_arcsec=0.400 sigma_q1_arcsec=0.355 sigma_q2_arcsec=0.419 sigma_q3_arcsec=0.438 sigma_q4_arcsec=0.426 n_q1=1232 n_q2=480 n_q3=935 n_q4=414 worst_quadrant_to_overall_ratio=1.095
The image catalog is written to wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits -region wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits sigma_overall=0.327 worst_q_ratio=1.093
ref2=Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits sigma_overall=0.360 worst_q_ratio=1.121
new1=fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits sigma_overall=0.414 worst_q_ratio=1.081
new2=fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits sigma_overall=0.400 worst_q_ratio=1.095
reference average sigma_overall=0.3435 worst_q_ratio=1.107
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387_astrometric_residuals.png (4771 matched stars from wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198_astrometric_residuals.png (4658 matched stars from wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268_astrometric_residuals.png (3196 matched stars from wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269_astrometric_residuals.png (3061 matched stars from wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits'
Saving fully-calibrated image wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits'
Preparing the HTML report for the field Aqr-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:26:38.61 -13:38:04.3: 15.44 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:26:38.61 -13:38:04.3: 15.47 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out22159.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
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 22158_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269
The candidate 22158_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269 did not pass the final checks
**** FOUND 21:02:32.76 -06:36:21.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22159_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269
Preparing report for the candidate 22159_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Aqr-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
21:26:38.61 -13:38:04.3
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
SExtractor catalog cache: saved Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.cat to cache
SExtractor catalog cache: saved Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
Creating symlink local_wcs_cache/wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits exists and is non-empty
wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits exists and is non-empty
wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits exists and is non-empty
wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits (1st reference image)
verification OK: wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
Image size: 937.4'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:25:43.484 -09:59:39.66 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits (1st new image)
verification OK: wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
Image size: 937.0'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:25:43.371 -09:59:43.71 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:25:43.484 -09:59:39.66
Second-epoch image center 21:25:43.371 -09:59:43.71
Angular distance between the image centers 0.0012 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits (2nd new image)
verification OK: wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
Image size: 937.0'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:25:40.380 -10:00:13.34 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:25:43.484 -09:59:39.66
Second-epoch image center 21:25:40.380 -10:00:13.34
Angular distance between the image centers 0.0158 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 21:25:43.371 -09:59:43.71
Second-epoch second image center 21:25:40.380 -10:00:13.34
Angular distance between the image centers 0.01478 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits &> /tmp/tmp.Y7v4cF9CGC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits &> /tmp/tmp.UGxc3rmPIA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits &> /tmp/tmp.yoOlnGwTH6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits &> /tmp/tmp.UHNp5N5tCj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits and wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits and wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat
Found non-empty wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits and wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat
The reference image (wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits) and catalog (wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat) found
'wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat' -> 'wcsmag.cat'
Read 53069 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.3814 to 329.5453 deg, Dec -15.2618 to -4.6695 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 313.3814 to 329.5453 deg, Dec -15.2618 to -4.6695 deg
Loaded 6771 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): 5405 out of 5966 total matches.
Matched with Tycho-2 5966 out of 53069 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.549900
a=0.000000 b=1.000000 c=22.549900
From vast_summary.log: estimated ref. image limiting mag.: -7.52
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.03
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.03
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 53069 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.3814 to 329.5453 deg, Dec -15.2618 to -4.6695 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 313.3814 to 329.5453 deg, Dec -15.2618 to -4.6695 deg
Loaded 6771 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): 5405 out of 5966 total matches.
Matched with Tycho-2 5966 out of 53069 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
Forced-photometry filter: calibrated wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits -> calib.txt_param_ref_wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits (aperture=4.9)
Read 51567 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.3495 to 329.5140 deg, Dec -15.2503 to -4.6788 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 313.3495 to 329.5140 deg, Dec -15.2503 to -4.6788 deg
Loaded 6759 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): 5424 out of 5938 total matches.
Matched with Tycho-2 5938 out of 51567 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
Forced-photometry filter: calibrated wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits -> calib.txt_param_ref_wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 22 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
2.3 pix Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
2.1 pix fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
2.1 pix fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
Limiting magnitude estimates:
15.0 mag. Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
15.0 mag. Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
14.3 mag. fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
14.2 mag. fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 13.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Y7v4cF9CGC (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits' -> 'wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
WCS_IMAGE_NAME=wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
WCS-calibrated image found: wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
Checking if the catalog wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat corresponding to the image wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits alredy exist and is non-empty...
Catalog wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat corresponding to the image wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
WCS catalog name: wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=2577, bad_region=7654, passed=53055
Got 53055 stars (including 43138 good ones) from the SExtractor catalog wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat
util/solve_plate_with_UCAC5 got 53055 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4798 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4784 matched stars entering correct_measured_positions(), 4784 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4783 matched stars entering correct_measured_positions(), 47298 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4798 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4782 matched stars entering correct_measured_positions(), 47298 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4782 matched stars entering correct_measured_positions(), 47298 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4782 stars left (next iteration limit 5261)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits N_match=4782 sigma_overall_arcsec=0.319 sigma_q1_arcsec=0.302 sigma_q2_arcsec=0.300 sigma_q3_arcsec=0.349 sigma_q4_arcsec=0.290 n_q1=1667 n_q2=781 n_q3=1558 n_q4=776 worst_quadrant_to_overall_ratio=1.092
The image catalog is written to wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits -region wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.UGxc3rmPIA (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits' -> 'wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
WCS_IMAGE_NAME=wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
WCS-calibrated image found: wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
Checking if the catalog wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat corresponding to the image wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits alredy exist and is non-empty...
Catalog wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat corresponding to the image wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
WCS catalog name: wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=3043, bad_region=10281, passed=51563
Got 51563 stars (including 39434 good ones) from the SExtractor catalog wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat
util/solve_plate_with_UCAC5 got 51563 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4673 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4654 matched stars entering correct_measured_positions(), 4654 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4654 matched stars entering correct_measured_positions(), 43678 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4673 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4654 matched stars entering correct_measured_positions(), 43678 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4654 matched stars entering correct_measured_positions(), 43678 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4654 stars left (next iteration limit 5119)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits N_match=4654 sigma_overall_arcsec=0.357 sigma_q1_arcsec=0.318 sigma_q2_arcsec=0.422 sigma_q3_arcsec=0.348 sigma_q4_arcsec=0.367 n_q1=1471 n_q2=857 n_q3=1384 n_q4=942 worst_quadrant_to_overall_ratio=1.182
The image catalog is written to wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits -region wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.yoOlnGwTH6 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
WCS-calibrated image found: wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
Checking if the catalog wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
WCS catalog name: wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1094, bad_region=4728, passed=32522
Got 32522 stars (including 26891 good ones) from the SExtractor catalog wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits.wcscat
util/solve_plate_with_UCAC5 got 32522 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4802 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4776 matched stars entering correct_measured_positions(), 4776 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4776 matched stars entering correct_measured_positions(), 28902 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4802 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4776 matched stars entering correct_measured_positions(), 28902 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4776 matched stars entering correct_measured_positions(), 28902 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4776 stars left (next iteration limit 5253)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits N_match=4776 sigma_overall_arcsec=0.405 sigma_q1_arcsec=0.376 sigma_q2_arcsec=0.431 sigma_q3_arcsec=0.425 sigma_q4_arcsec=0.407 n_q1=1805 n_q2=688 n_q3=1598 n_q4=685 worst_quadrant_to_overall_ratio=1.065
The image catalog is written to wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits -region wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.UHNp5N5tCj (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
WCS-calibrated image found: wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
Checking if the catalog wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
WCS catalog name: wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=1123, bad_region=4307, passed=31635
Got 31635 stars (including 26417 good ones) from the SExtractor catalog wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits.wcscat
util/solve_plate_with_UCAC5 got 31635 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4804 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4778 matched stars entering correct_measured_positions(), 4779 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4778 matched stars entering correct_measured_positions(), 28269 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4804 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4779 matched stars entering correct_measured_positions(), 28269 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4779 matched stars entering correct_measured_positions(), 28269 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4779 stars left (next iteration limit 5255)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits N_match=4779 sigma_overall_arcsec=0.405 sigma_q1_arcsec=0.368 sigma_q2_arcsec=0.401 sigma_q3_arcsec=0.449 sigma_q4_arcsec=0.390 n_q1=1859 n_q2=697 n_q3=1555 n_q4=668 worst_quadrant_to_overall_ratio=1.110
The image catalog is written to wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits -region wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-38-06_20.00sec_-0.00C_LIGHT_0268.fits
Saving fully-calibrated image wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aqr-03-Q2b1x1_021719_TTUQ2b1x1_2636542_NfXbDpSD/wcs_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269.fits
Preparing the HTML report for the field Aqr-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:02:08.29 -12:31:52.2: 13.58 +/- 0.06 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:36:08.53 -07:32:46.5: 13.18 +/- 0.04 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:17:23.57 -10:32:58.1: 12.55 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 20:57:56.23 -08:21:40.2: 13.08 +/- 0.04 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:38:57.31 -08:15:19.2: 12.84 +/- 0.03 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:35:42.93 -12:37:07.7: 13.47 +/- 0.05 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:08:34.53 -06:47:42.6: 12.60 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:34:16.32 -06:17:44.4: 11.34 +/- 0.01 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:21:52.30 -07:26:13.9: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:19:12.54 -11:39:09.6: 15.60 +/- 0.34 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:02:08.29 -12:31:52.2: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:17:23.57 -10:32:58.1: 12.43 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:38:57.31 -08:15:19.2: 12.76 +/- 0.03 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:08:34.53 -06:47:42.6: 12.35 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:36:08.53 -07:32:46.5: 13.14 +/- 0.04 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 20:57:56.23 -08:21:40.2: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:34:16.32 -06:17:44.4: 11.31 +/- 0.01 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:21:52.30 -07:26:13.9: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:35:42.93 -12:37:07.7: 13.35 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.06
Forced photometry reference-image weighted average: 13.08 +/- 0.04
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Forced photometry filter REJECTED candidate at 21:02:08.29 -12:31:52.2: ref_mag=13.58 +/- 0.06 new_mean_mag=13.8914 delta=-0.32 (need > 0.90)
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Forced photometry reference-image weighted average: 13.16 +/- 0.03
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Forced photometry reference-image weighted average: 11.33 +/- 0.00
Forced photometry filter REJECTED candidate at 21:17:23.57 -10:32:58.1: ref_mag=12.48 +/- 0.01 new_mean_mag=12.6412 delta=-0.16 (need > 0.90)
Forced photometry filter REJECTED candidate at 20:57:56.23 -08:21:40.2: ref_mag=13.08 +/- 0.04 new_mean_mag=13.2396 delta=-0.16 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:38:57.31 -08:15:19.2: ref_mag=12.80 +/- 0.02 new_mean_mag=12.9075 delta=-0.11 (need > 0.90)
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Forced photometry filter REJECTED candidate at 21:08:34.53 -06:47:42.6: ref_mag=12.44 +/- 0.01 new_mean_mag=12.8215 delta=-0.38 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:36:08.53 -07:32:46.5: ref_mag=13.16 +/- 0.03 new_mean_mag=13.3723 delta=-0.21 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:34:16.32 -06:17:44.4: ref_mag=11.33 +/- 0.00 new_mean_mag=11.5402 delta=-0.21 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:35:42.93 -12:37:07.7: ref_mag=13.40 +/- 0.03 new_mean_mag=13.7857 delta=-0.38 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:19:12.54 -11:39:09.6: 15.66 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.60 +/- 0.34
Forced photometry filter KEPT candidate at 21:19:12.54 -11:39:09.6: ref_mag=15.60 +/- 0.34 new_mean_mag=12.4658 delta=3.14 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:20:16.01 -10:35:25.0: 13.28 +/- 0.04 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:32:22.71 -12:17:26.7: 13.17 +/- 0.05 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:09:44.91 -11:22:06.3: 13.34 +/- 0.06 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:07:12.15 -09:46:34.4: 13.44 +/- 0.05 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:02:22.13 -09:41:24.4: 13.31 +/- 0.05 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:13:52.26 -11:56:15.6: 13.39 +/- 0.05 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:20:00.72 -13:55:00.6: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:33:29.07 -13:26:49.4: 13.36 +/- 0.06 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:20:16.01 -10:35:25.0: 13.26 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Forced photometry filter REJECTED candidate at 21:20:16.01 -10:35:25.0: ref_mag=13.27 +/- 0.03 new_mean_mag=13.3658 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:13:52.26 -11:56:15.6: 13.48 +/- 0.05 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:07:12.15 -09:46:34.4: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:02:22.13 -09:41:24.4: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:32:22.71 -12:17:26.7: 13.14 +/- 0.04 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:09:44.91 -11:22:06.3: 13.49 +/- 0.06 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:20:00.72 -13:55:00.6: 15.60 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.43 +/- 0.04
Forced photometry reference-image weighted average: 13.44 +/- 0.05
Forced photometry reference-image weighted average: 13.31 +/- 0.05
Forced photometry reference-image weighted average: 13.15 +/- 0.03
Forced photometry filter REJECTED candidate at 21:13:52.26 -11:56:15.6: ref_mag=13.43 +/- 0.04 new_mean_mag=13.3772 delta=0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:02:22.13 -09:41:24.4: ref_mag=13.31 +/- 0.05 new_mean_mag=13.2253 delta=0.09 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:32:22.71 -12:17:26.7: ref_mag=13.15 +/- 0.03 new_mean_mag=13.3238 delta=-0.17 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:07:12.15 -09:46:34.4: ref_mag=13.44 +/- 0.05 new_mean_mag=13.2626 delta=0.18 (need > 0.90)
Forced photometry reference-image weighted average: 13.41 +/- 0.04
Forced photometry filter REJECTED candidate at 21:09:44.91 -11:22:06.3: ref_mag=13.41 +/- 0.04 new_mean_mag=13.4000 delta=0.01 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:33:29.07 -13:26:49.4: 13.32 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.04
Forced photometry filter REJECTED candidate at 21:33:29.07 -13:26:49.4: ref_mag=13.34 +/- 0.04 new_mean_mag=13.5749 delta=-0.24 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 20:59:25.43 -09:01:53.2: 14.57 +/- 0.15 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 20:59:25.43 -09:01:53.2: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 14.57 +/- 0.15
Forced photometry filter REJECTED candidate at 20:59:25.43 -09:01:53.2: ref_mag=14.57 +/- 0.15 new_mean_mag=14.3550 delta=0.21 (need > 0.90)
Adding exclusion_list_local.txt__out75002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75008.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75019.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 74963_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269
The candidate 74963_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269 did not pass the final checks
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Considering the candidate 74968_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269
The candidate 74968_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269 did not pass the final checks
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Considering the candidate 74975_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269
The candidate 74975_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269 did not pass the final checks
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Considering the candidate 74981_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269
The candidate 74981_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269 did not pass the final checks
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Considering the candidate 74985_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269
The candidate 74985_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269 did not pass the final checks
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Considering the candidate 74989_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269
The candidate 74989_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269 did not pass the final checks
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Considering the candidate 74991_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269
The candidate 74991_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269 did not pass the final checks
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Considering the candidate 74994_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269
The candidate 74994_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269 did not pass the final checks
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Considering the candidate 74997_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269
The candidate 74997_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269 did not pass the final checks
**** FOUND 21:26:38.60 -13:38:04.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 75002_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269
Preparing report for the candidate 75002_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269
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Considering the candidate 75008_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269
Preparing report for the candidate 75008_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269
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Considering the candidate 75018_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269
The candidate 75018_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269 did not pass the final checks
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Considering the candidate 75019_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269
Preparing report for the candidate 75019_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269
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Considering the candidate 75022_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269
The candidate 75022_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269 did not pass the final checks
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Considering the candidate 75023_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269
The candidate 75023_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 75028_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269
The candidate 75028_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269 did not pass the final checks
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Considering the candidate 75029_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269
The candidate 75029_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269 did not pass the final checks
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Considering the candidate 75031_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269
The candidate 75031_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269 did not pass the final checks
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Considering the candidate 75037_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269
The candidate 75037_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269 did not pass the final checks
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Considering the candidate 75048_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269
The candidate 75048_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269 did not pass the final checks
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Considering the candidate 75092_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269
The candidate 75092_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269 did not pass the final checks
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Considering the candidate 45096_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269
The candidate 45096_fd_Aqr-03-Q2b1x1_2026-08-06_01-39-01_20.00sec_-0.00C_LIGHT_0269 did not pass the final checks