This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 10 12.1978 2461325.6978 11.62 23:10:27.86 -20:03:05.7
44.53989 -65.85930 galactic Aqr Second-epoch detections are separated by 0.7" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.23 Thalia 0 -0 0 11.9 0 0
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:10:27.86 -20:03:05.7: 15.01 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:10:27.86 -20:03:05.7: 14.79 +/- 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,2461325.6978,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261012.1978 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 12.1978 2461325.6978 12.20 23:22:29.78 -14:21:45.0
60.09698 -65.66725 galactic Aqr Second-epoch detections are separated by 0.8" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.118 Peitho -1 -0 1 12.3 0 -0
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:22:29.78 -14:21:45.0: 14.97 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:22:29.78 -14:21:45.0: 14.82 +/- 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,2461325.6978,12.20,0.05,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 20261012.1978 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 12.1978 2461325.6978 13.19 23:12:26.99 -15:30:55.0
54.68521 -64.26025 galactic Aqr Second-epoch detections are separated by 0.5" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.530 Turandot -0 0 0 13.3 -0 -0
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:12:26.99 -15:30:55.0: 15.10 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:12:26.99 -15:30:55.0: 14.89 +/- 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,2461325.6978,13.19,0.05,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 20261012.1978 13.19CV 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: 2461212.88469579 21.06.2026 09:13:47.716 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
First image: 2461212.88469579 21.06.2026 09:13:47.716 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
Last image: 2461325.69814667 12.10.2026 04:45:09.872 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.94
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): 4246
Objects passed selection criteria: 4231
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 3089.5
Average stars matched: 2554.5 (82.6833 %)
Memory usage VmPeak: 230608 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Oct 9 16:07:04 CDT 2026
VaST build number 1.0rc89-234-g1a8c12b2
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-09)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Oct 12 00:16:35 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: 2461212.88469579 21.06.2026 09:13:47.716 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
First image: 2461212.88469579 21.06.2026 09:13:47.716 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
Last image: 2461325.69814667 12.10.2026 04:45:09.872 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 82
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
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: 15 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): 24212
Objects passed selection criteria: 24148
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: 18806.8
Average stars matched: 15819.2 (84.1147 %)
Memory usage VmPeak: 246172 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Oct 9 16:07:04 CDT 2026
VaST build number 1.0rc89-234-g1a8c12b2
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-09)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Oct 12 00:19:39 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
SExtractor catalog cache: saved Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.cat to cache
SExtractor catalog cache: saved Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.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-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461325.69739678
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits exists and is non-empty
wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits exists and is non-empty
wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits exists and is non-empty
wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits (1st reference image)
verification OK: wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
Image size: 937.7'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 23:06:40.465 -17:59:46.14 J2000 4789.000 3195.000
###################################
The image scale is 5.88"/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-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits (1st new image)
verification OK: wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
Image size: 936.9'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: 23:06:40.622 -17:59:45.48 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:06:40.465 -17:59:46.14
Second-epoch image center 23:06:40.622 -17:59:45.48
Angular distance between the image centers 0.0006 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits (2nd new image)
verification OK: wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
Image size: 936.9'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: 23:06:38.062 -18:00:13.75 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:06:40.465 -17:59:46.14
Second-epoch image center 23:06:38.062 -18:00:13.75
Angular distance between the image centers 0.0122 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 23:06:40.622 -17:59:45.48
Second-epoch second image center 23:06:38.062 -18:00:13.75
Angular distance between the image centers 0.01283 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-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits &> /tmp/tmp.PHA0xBrSkI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits &> /tmp/tmp.pXFNCn4pD4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits &> /tmp/tmp.euHIwcsfIA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits &> /tmp/tmp.2CMNpukXNV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.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-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits and wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
'tns_transients_list.txt' -> '../tns_transients_list.txt'
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-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits and wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat
Found non-empty wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits and wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat
The reference image (wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits) and catalog (wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat) found
'wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat' -> 'wcsmag.cat'
Read 3335 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.2681 to 355.1405 deg, Dec -23.2523 to -12.5761 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 338.2681 to 355.1405 deg, Dec -23.2523 to -12.5761 deg
Loaded 4546 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): 2669 out of 2711 total matches.
Matched with Tycho-2 2711 out of 3335 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.435500
a=0.000000 b=1.000000 c=22.435500
From vast_summary.log: estimated ref. image limiting mag.: -7.94
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.50
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.50
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 3335 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.2681 to 355.1405 deg, Dec -23.2523 to -12.5761 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 338.2681 to 355.1405 deg, Dec -23.2523 to -12.5761 deg
Loaded 4546 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): 2669 out of 2711 total matches.
Matched with Tycho-2 2711 out of 3335 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
Forced-photometry filter: calibrated wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits -> calib.txt_param_ref_wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits (aperture=6.2)
Read 2735 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.2677 to 355.1377 deg, Dec -23.2523 to -12.5973 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 338.2677 to 355.1377 deg, Dec -23.2523 to -12.5973 deg
Loaded 4533 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): 2231 out of 2254 total matches.
Matched with Tycho-2 2254 out of 2735 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
Forced-photometry filter: calibrated wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits -> calib.txt_param_ref_wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
2.2 pix Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
2.2 pix fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
2.2 pix fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
Limiting magnitude estimates:
14.5 mag. Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
14.3 mag. Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
15.1 mag. fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
15.1 mag. fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
All-image limiting magnitude estimate: 15.1 (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
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.PHA0xBrSkI (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.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-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits' -> 'wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.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-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
WCS_IMAGE_NAME=wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
WCS-calibrated image found: wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
Checking if the catalog wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat corresponding to the image wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits alredy exist and is non-empty...
Catalog wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat corresponding to the image wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
WCS catalog name: wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.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=238, bad_region=696, passed=3335
Got 3335 stars (including 2446 good ones) from the SExtractor catalog wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat
util/solve_plate_with_UCAC5 got 3335 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 2317 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2312 matched stars entering correct_measured_positions(), 2312 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2312 matched stars entering correct_measured_positions(), 2761 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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 2317 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2311 matched stars entering correct_measured_positions(), 2761 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 2311 matched stars entering correct_measured_positions(), 2760 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 2311 stars left (next iteration limit 2543)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits N_match=2311 sigma_overall_arcsec=0.367 sigma_q1_arcsec=0.352 sigma_q2_arcsec=0.340 sigma_q3_arcsec=0.390 sigma_q4_arcsec=0.350 n_q1=783 n_q2=386 n_q3=710 n_q4=432 worst_quadrant_to_overall_ratio=1.064
The image catalog is written to wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits -region wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.pXFNCn4pD4 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.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-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits' -> 'wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.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-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
WCS_IMAGE_NAME=wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
WCS-calibrated image found: wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
Checking if the catalog wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat corresponding to the image wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits alredy exist and is non-empty...
Catalog wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat corresponding to the image wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
WCS catalog name: wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.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=193, bad_region=579, passed=2735
Got 2735 stars (including 2002 good ones) from the SExtractor catalog wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat
util/solve_plate_with_UCAC5 got 2735 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 1902 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1900 matched stars entering correct_measured_positions(), 1900 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1900 matched stars entering correct_measured_positions(), 2242 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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 1902 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1900 matched stars entering correct_measured_positions(), 2242 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 1900 matched stars entering correct_measured_positions(), 2242 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 1900 stars left (next iteration limit 2090)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits N_match=1900 sigma_overall_arcsec=0.387 sigma_q1_arcsec=0.325 sigma_q2_arcsec=0.356 sigma_q3_arcsec=0.471 sigma_q4_arcsec=0.344 n_q1=625 n_q2=315 n_q3=613 n_q4=347 worst_quadrant_to_overall_ratio=1.217
The image catalog is written to wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits -region wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.euHIwcsfIA (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
WCS-calibrated image found: wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
Checking if the catalog wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits.wcscat corresponding to the image wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits.wcscat corresponding to the image wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
WCS catalog name: wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.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=321, bad_region=1261, passed=5069
Got 5069 stars (including 3546 good ones) from the SExtractor catalog wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits.wcscat
util/solve_plate_with_UCAC5 got 5069 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 333 to 388 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 3415 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3411 matched stars entering correct_measured_positions(), 3411 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3411 matched stars entering correct_measured_positions(), 4033 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 333 to 388 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 3415 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3411 matched stars entering correct_measured_positions(), 4033 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 3411 matched stars entering correct_measured_positions(), 4033 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 3411 stars left (next iteration limit 3752)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3411 robust_rms=7.421 arcsec worst_region_rms=16.234 arcsec outer_annulus_rms=16.234 arcsec
SIP_REFIT: SIP order 3 trial: matched=3411 robust_rms=0.384 arcsec worst_region_rms=0.758 arcsec outer_annulus_rms=0.758 arcsec
SIP_REFIT: SIP order 5 trial: matched=3411 robust_rms=0.312 arcsec worst_region_rms=0.374 arcsec outer_annulus_rms=0.374 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3411 robust_rms_before=0.925 arcsec robust_rms_before_corrected=0.319 arcsec robust_rms_after=0.312 arcsec worst_region_rms_before=0.379 worst_region_rms_after=0.374 outer_annulus_rms_before=1.367 outer_annulus_rms_after=0.374
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.379 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits worst_region_rms_kept=0.379 arcsec robust_rms_kept=0.319 arcsec matched=3411
WCS_QUALITY_DIAG: file=fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits N_match=3411 sigma_overall_arcsec=0.328 sigma_q1_arcsec=0.311 sigma_q2_arcsec=0.357 sigma_q3_arcsec=0.324 sigma_q4_arcsec=0.308 n_q1=1090 n_q2=677 n_q3=999 n_q4=645 worst_quadrant_to_overall_ratio=1.091
The image catalog is written to wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits -region wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.2CMNpukXNV (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
WCS-calibrated image found: wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
Checking if the catalog wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits.wcscat corresponding to the image wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits.wcscat corresponding to the image wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
WCS catalog name: wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.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=315, bad_region=1249, passed=5070
Got 5070 stars (including 3567 good ones) from the SExtractor catalog wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits.wcscat
util/solve_plate_with_UCAC5 got 5070 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 333 to 388 (Dec -23.3 to -12.7)
Done reading UCAC5 zone files...
Matched 3438 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3433 matched stars entering correct_measured_positions(), 3433 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3433 matched stars entering correct_measured_positions(), 4049 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 333 to 388 (Dec -23.3 to -12.7)
Done reading UCAC5 zone files...
Matched 3438 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3433 matched stars entering correct_measured_positions(), 4049 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 3433 matched stars entering correct_measured_positions(), 4049 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 3433 stars left (next iteration limit 3776)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3433 robust_rms=7.509 arcsec worst_region_rms=16.258 arcsec outer_annulus_rms=16.258 arcsec
SIP_REFIT: SIP order 3 trial: matched=3433 robust_rms=0.373 arcsec worst_region_rms=0.667 arcsec outer_annulus_rms=0.667 arcsec
SIP_REFIT: SIP order 5 trial: matched=3433 robust_rms=0.300 arcsec worst_region_rms=0.370 arcsec outer_annulus_rms=0.370 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3433 robust_rms_before=0.932 arcsec robust_rms_before_corrected=0.302 arcsec robust_rms_after=0.300 arcsec worst_region_rms_before=0.367 worst_region_rms_after=0.370 outer_annulus_rms_before=1.319 outer_annulus_rms_after=0.370
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.367 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits worst_region_rms_kept=0.367 arcsec robust_rms_kept=0.302 arcsec matched=3433
WCS_QUALITY_DIAG: file=fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits N_match=3433 sigma_overall_arcsec=0.315 sigma_q1_arcsec=0.286 sigma_q2_arcsec=0.351 sigma_q3_arcsec=0.305 sigma_q4_arcsec=0.334 n_q1=1092 n_q2=667 n_q3=1013 n_q4=661 worst_quadrant_to_overall_ratio=1.115
The image catalog is written to wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits -region wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits to local_wcs_cache/
'wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits' -> 'local_wcs_cache/wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits'
Saving the final (post-refit) wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits to local_wcs_cache/
'wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits' -> 'local_wcs_cache/wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits'
Saving the final (post-refit) wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits to local_wcs_cache/
'wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits' -> 'local_wcs_cache/wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits'
Saving the final (post-refit) wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits to local_wcs_cache/
'wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits' -> 'local_wcs_cache/wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits sigma_overall=0.367 worst_q_ratio=1.064
ref2=Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits sigma_overall=0.387 worst_q_ratio=1.217
new1=fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits sigma_overall=0.328 worst_q_ratio=1.091
new2=fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits sigma_overall=0.315 worst_q_ratio=1.115
reference average sigma_overall=0.377 worst_q_ratio=1.1405
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406_astrometric_residuals.png (2311 matched stars from wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410_astrometric_residuals.png (1900 matched stars from wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248_astrometric_residuals.png (3411 matched stars from wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249_astrometric_residuals.png (3433 matched stars from wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits'
Saving fully-calibrated image wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits'
Preparing the HTML report for the field Aqr-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 22:58:13.84 -17:42:22.1: 11.21 +/- 0.01 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:01:14.29 -19:09:54.6: 11.33 +/- 0.01 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:05:17.13 -16:51:39.5: 11.19 +/- 0.01 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:03:13.55 -17:24:03.5: 11.24 +/- 0.01 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 22:58:13.84 -17:42:22.1: 11.23 +/- 0.01 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:01:14.29 -19:09:54.6: 11.35 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.21 +/- 0.01
Forced photometry filter REJECTED candidate at 22:58:13.84 -17:42:22.1: ref_mag=11.21 +/- 0.01 new_mean_mag=11.2270 delta=-0.01 (need > 0.90)
Forced photometry reference-image weighted average: 11.34 +/- 0.01
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:05:17.13 -16:51:39.5: 11.21 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 23:01:14.29 -19:09:54.6: ref_mag=11.34 +/- 0.01 new_mean_mag=11.3183 delta=0.02 (need > 0.90)
Forced photometry reference-image weighted average: 11.20 +/- 0.01
Forced photometry filter REJECTED candidate at 23:05:17.13 -16:51:39.5: ref_mag=11.20 +/- 0.01 new_mean_mag=11.1671 delta=0.03 (need > 0.90)
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:03:13.55 -17:24:03.5: 11.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.24 +/- 0.01
Forced photometry filter REJECTED candidate at 23:03:13.55 -17:24:03.5: ref_mag=11.24 +/- 0.01 new_mean_mag=11.2513 delta=-0.01 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20318_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 20318_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
**** FOUND 23:04:00.59 -20:54:22.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20426_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 20426_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20447_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 20447_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20465_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 20465_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20492_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 20492_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00931_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 00931_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
**** FOUND 22:57:06.61 -20:20:35.0 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Aqr-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
SExtractor catalog cache: saved Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.cat to cache
SExtractor catalog cache: saved Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.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-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
Creating symlink local_wcs_cache/wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits exists and is non-empty
wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits exists and is non-empty
wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits exists and is non-empty
wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits (1st reference image)
verification OK: wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
Image size: 937.7'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 23:06:40.465 -17:59:46.14 J2000 4789.000 3195.000
###################################
The image scale is 5.88"/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-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits (1st new image)
verification OK: wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
Image size: 936.9'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: 23:06:40.622 -17:59:45.48 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:06:40.465 -17:59:46.14
Second-epoch image center 23:06:40.622 -17:59:45.48
Angular distance between the image centers 0.0006 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits (2nd new image)
verification OK: wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
Image size: 936.9'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: 23:06:38.062 -18:00:13.75 J2000 4789.000 3195.000
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###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:06:40.465 -17:59:46.14
Second-epoch image center 23:06:38.062 -18:00:13.75
Angular distance between the image centers 0.0122 deg.
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###################################
# 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 23:06:40.622 -17:59:45.48
Second-epoch second image center 23:06:38.062 -18:00:13.75
Angular distance between the image centers 0.01283 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-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits &> /tmp/tmp.AjAxobmKMF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits &> /tmp/tmp.QKhufBPQK0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits &> /tmp/tmp.d0GOWrLqyZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits &> /tmp/tmp.ecASAn8vYr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.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-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits and wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.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-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits and wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat
Found non-empty wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits and wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat
The reference image (wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits) and catalog (wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat) found
'wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat' -> 'wcsmag.cat'
Read 19454 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.2356 to 355.1719 deg, Dec -23.2559 to -12.5761 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 338.2356 to 355.1719 deg, Dec -23.2559 to -12.5761 deg
Loaded 4568 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): 3693 out of 3823 total matches.
Matched with Tycho-2 3823 out of 19454 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.293600
a=0.000000 b=1.000000 c=22.293600
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.67
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.67
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 19454 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.2356 to 355.1719 deg, Dec -23.2559 to -12.5761 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 338.2356 to 355.1719 deg, Dec -23.2559 to -12.5761 deg
Loaded 4568 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): 3693 out of 3823 total matches.
Matched with Tycho-2 3823 out of 19454 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
Forced-photometry filter: calibrated wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits -> calib.txt_param_ref_wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits (aperture=4.8)
Read 17815 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.2344 to 355.1739 deg, Dec -23.2554 to -12.5760 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 338.2344 to 355.1739 deg, Dec -23.2554 to -12.5760 deg
Loaded 4568 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): 3728 out of 3836 total matches.
Matched with Tycho-2 3836 out of 17815 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
Forced-photometry filter: calibrated wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits -> calib.txt_param_ref_wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 34 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
2.1 pix Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
2.1 pix fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
2.1 pix fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
Limiting magnitude estimates:
14.7 mag. Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
14.5 mag. Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
15.2 mag. fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
15.2 mag. fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 13.8 (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.AjAxobmKMF (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.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-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits' -> 'wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.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-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
WCS_IMAGE_NAME=wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
WCS-calibrated image found: wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
Checking if the catalog wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat corresponding to the image wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits alredy exist and is non-empty...
Catalog wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat corresponding to the image wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
WCS catalog name: wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.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=650, bad_region=2800, passed=19446
Got 19446 stars (including 16167 good ones) from the SExtractor catalog wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat
util/solve_plate_with_UCAC5 got 19446 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4784 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(), 4778 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4778 matched stars entering correct_measured_positions(), 17350 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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4784 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4778 matched stars entering correct_measured_positions(), 17350 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4778 matched stars entering correct_measured_positions(), 17350 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4778 stars left (next iteration limit 5255)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits N_match=4778 sigma_overall_arcsec=0.379 sigma_q1_arcsec=0.367 sigma_q2_arcsec=0.392 sigma_q3_arcsec=0.389 sigma_q4_arcsec=0.362 n_q1=1568 n_q2=774 n_q3=1522 n_q4=914 worst_quadrant_to_overall_ratio=1.034
The image catalog is written to wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits -region wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.QKhufBPQK0 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.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-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits' -> 'wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.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-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
WCS_IMAGE_NAME=wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
WCS-calibrated image found: wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
Checking if the catalog wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat corresponding to the image wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits alredy exist and is non-empty...
Catalog wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat corresponding to the image wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
WCS catalog name: wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.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=542, bad_region=2798, passed=17807
Got 17807 stars (including 14549 good ones) from the SExtractor catalog wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat
util/solve_plate_with_UCAC5 got 17807 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4789 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4782 matched stars entering correct_measured_positions(), 4782 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4782 matched stars entering correct_measured_positions(), 15700 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4789 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(), 15700 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4782 matched stars entering correct_measured_positions(), 15700 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 4782 stars left (next iteration limit 5260)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits N_match=4782 sigma_overall_arcsec=0.415 sigma_q1_arcsec=0.392 sigma_q2_arcsec=0.423 sigma_q3_arcsec=0.469 sigma_q4_arcsec=0.368 n_q1=1572 n_q2=818 n_q3=1474 n_q4=918 worst_quadrant_to_overall_ratio=1.130
The image catalog is written to wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits -region wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.d0GOWrLqyZ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
WCS-calibrated image found: wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
Checking if the catalog wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits.wcscat corresponding to the image wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits.wcscat corresponding to the image wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
WCS catalog name: wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=967, bad_region=5103, passed=27208
Got 27208 stars (including 21422 good ones) from the SExtractor catalog wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits.wcscat
util/solve_plate_with_UCAC5 got 27208 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 333 to 388 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4840 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4836 matched stars entering correct_measured_positions(), 4836 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4836 matched stars entering correct_measured_positions(), 23322 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 333 to 388 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4838 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4835 matched stars entering correct_measured_positions(), 23322 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4835 matched stars entering correct_measured_positions(), 23322 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4835 stars left (next iteration limit 5319)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4835 robust_rms=7.210 arcsec worst_region_rms=14.501 arcsec outer_annulus_rms=14.501 arcsec
SIP_REFIT: SIP order 3 trial: matched=4835 robust_rms=0.394 arcsec worst_region_rms=0.717 arcsec outer_annulus_rms=0.717 arcsec
SIP_REFIT: SIP order 5 trial: matched=4835 robust_rms=0.323 arcsec worst_region_rms=0.391 arcsec outer_annulus_rms=0.391 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4835 robust_rms_before=0.922 arcsec robust_rms_before_corrected=0.321 arcsec robust_rms_after=0.323 arcsec worst_region_rms_before=0.380 worst_region_rms_after=0.391 outer_annulus_rms_before=1.327 outer_annulus_rms_after=0.391
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.380 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits worst_region_rms_kept=0.380 arcsec robust_rms_kept=0.321 arcsec matched=4835
WCS_QUALITY_DIAG: file=fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits N_match=4835 sigma_overall_arcsec=0.334 sigma_q1_arcsec=0.321 sigma_q2_arcsec=0.337 sigma_q3_arcsec=0.327 sigma_q4_arcsec=0.338 n_q1=1552 n_q2=917 n_q3=1484 n_q4=882 worst_quadrant_to_overall_ratio=1.013
The image catalog is written to wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits -region wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.ecASAn8vYr (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
WCS-calibrated image found: wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
Checking if the catalog wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits.wcscat corresponding to the image wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits.wcscat corresponding to the image wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
WCS catalog name: wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.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=11, blended=996, bad_region=5106, passed=27105
Got 27105 stars (including 21316 good ones) from the SExtractor catalog wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits.wcscat
util/solve_plate_with_UCAC5 got 27105 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 333 to 388 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4840 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4837 matched stars entering correct_measured_positions(), 4837 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4837 matched stars entering correct_measured_positions(), 23191 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4839 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4837 matched stars entering correct_measured_positions(), 23191 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4837 matched stars entering correct_measured_positions(), 23191 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4837 stars left (next iteration limit 5320)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4837 robust_rms=7.272 arcsec worst_region_rms=14.483 arcsec outer_annulus_rms=14.483 arcsec
SIP_REFIT: SIP order 3 trial: matched=4837 robust_rms=0.392 arcsec worst_region_rms=0.641 arcsec outer_annulus_rms=0.641 arcsec
SIP_REFIT: SIP order 5 trial: matched=4837 robust_rms=0.307 arcsec worst_region_rms=0.367 arcsec outer_annulus_rms=0.367 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4837 robust_rms_before=0.930 arcsec robust_rms_before_corrected=0.303 arcsec robust_rms_after=0.307 arcsec worst_region_rms_before=0.367 worst_region_rms_after=0.367 outer_annulus_rms_before=1.288 outer_annulus_rms_after=0.367
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.367 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits worst_region_rms_kept=0.367 arcsec robust_rms_kept=0.303 arcsec matched=4837
WCS_QUALITY_DIAG: file=fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits N_match=4837 sigma_overall_arcsec=0.312 sigma_q1_arcsec=0.286 sigma_q2_arcsec=0.330 sigma_q3_arcsec=0.325 sigma_q4_arcsec=0.309 n_q1=1558 n_q2=904 n_q3=1482 n_q4=893 worst_quadrant_to_overall_ratio=1.057
The image catalog is written to wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits -region wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-44-05_20.00sec_0.00C_LIGHT_0248.fits
Saving fully-calibrated image wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Aqr-07-Q2b1x1_001047_TTUQ2b1x1_1140252_ptWXEWKD/wcs_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249.fits
Preparing the HTML report for the field Aqr-07-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:22:29.78 -14:21:45.0: 14.97 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:25:46.36 -20:37:47.1: 13.84 +/- 0.18 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:12:26.99 -15:30:55.0: 15.10 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:23:26.20 -21:30:31.4: 13.83 +/- 0.16 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:23:57.54 -21:34:31.5: 13.73 +/- 0.13 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:24:11.67 -14:55:24.9: 13.24 +/- 0.08 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:10:27.86 -20:03:05.7: 15.01 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:19:38.05 -22:10:22.5: 14.00 +/- 0.17 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:25:14.31 -21:31:56.8: 13.78 +/- 0.15 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:22:44.62 -20:49:22.8: 14.15 +/- 0.18 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:19:38.05 -22:10:22.5: 13.68 +/- 0.15 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:22:29.78 -14:21:45.0: 14.82 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:23:26.20 -21:30:31.4: 13.84 +/- 0.18 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:10:27.86 -20:03:05.7: 14.79 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:24:11.67 -14:55:24.9: 13.23 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.11
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:25:46.36 -20:37:47.1: 14.06 +/- 0.27 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:12:26.99 -15:30:55.0: 14.89 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.83 +/- 0.12
Forced photometry filter REJECTED candidate at 23:19:38.05 -22:10:22.5: ref_mag=13.83 +/- 0.11 new_mean_mag=13.8650 delta=-0.04 (need > 0.90)
Forced photometry reference-image weighted average: 13.24 +/- 0.06
Forced photometry filter REJECTED candidate at 23:23:26.20 -21:30:31.4: ref_mag=13.83 +/- 0.12 new_mean_mag=13.7699 delta=0.06 (need > 0.90)
Forced photometry reference-image weighted average: 13.91 +/- 0.15
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:23:57.54 -21:34:31.5: 13.62 +/- 0.14 detection
Forced photometry filter REJECTED candidate at 23:25:46.36 -20:37:47.1: ref_mag=13.91 +/- 0.15 new_mean_mag=13.8491 delta=0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:24:11.67 -14:55:24.9: ref_mag=13.24 +/- 0.06 new_mean_mag=13.3484 delta=-0.11 (need > 0.90)
Forced photometry reference-image weighted average: 13.68 +/- 0.10
Forced photometry filter REJECTED candidate at 23:23:57.54 -21:34:31.5: ref_mag=13.68 +/- 0.10 new_mean_mag=13.8977 delta=-0.22 (need > 0.90)
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:25:14.31 -21:31:56.8: 13.97 +/- 0.20 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.12
Forced photometry filter REJECTED candidate at 23:25:14.31 -21:31:56.8: ref_mag=13.85 +/- 0.12 new_mean_mag=13.8234 delta=0.02 (need > 0.90)
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:22:44.62 -20:49:22.8: 13.94 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.05 +/- 0.13
Forced photometry filter REJECTED candidate at 23:22:44.62 -20:49:22.8: ref_mag=14.05 +/- 0.13 new_mean_mag=13.7965 delta=0.25 (need > 0.90)
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:25:51.98 -21:49:28.0: 13.71 +/- 0.14 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:23:55.41 -21:11:05.4: 14.24 +/- 0.22 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:25:40.41 -21:12:48.7: 13.93 +/- 0.17 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:21:30.69 -20:31:33.7: 14.08 +/- 0.18 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:19:14.87 -21:53:17.7: 14.19 +/- 0.20 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:25:54.64 -21:47:12.9: 14.03 +/- 0.19 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:21:52.32 -21:42:40.0: 13.96 +/- 0.16 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:25:51.98 -21:49:28.0: 13.90 +/- 0.19 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.11
Forced photometry filter REJECTED candidate at 23:25:51.98 -21:49:28.0: ref_mag=13.78 +/- 0.11 new_mean_mag=13.8497 delta=-0.07 (need > 0.90)
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:23:55.41 -21:11:05.4: 13.89 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.14
Forced photometry filter REJECTED candidate at 23:23:55.41 -21:11:05.4: ref_mag=14.04 +/- 0.14 new_mean_mag=13.9913 delta=0.04 (need > 0.90)
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:21:30.69 -20:31:33.7: 14.16 +/- 0.21 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:25:40.41 -21:12:48.7: 14.02 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.14
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:19:14.87 -21:53:17.7: 13.65 +/- 0.14 detection
Forced photometry filter REJECTED candidate at 23:21:30.69 -20:31:33.7: ref_mag=14.12 +/- 0.14 new_mean_mag=13.9648 delta=0.15 (need > 0.90)
Forced photometry reference-image weighted average: 13.97 +/- 0.13
Forced photometry filter REJECTED candidate at 23:25:40.41 -21:12:48.7: ref_mag=13.97 +/- 0.13 new_mean_mag=13.8924 delta=0.07 (need > 0.90)
Forced photometry reference-image weighted average: 13.84 +/- 0.11
Forced photometry filter REJECTED candidate at 23:19:14.87 -21:53:17.7: ref_mag=13.84 +/- 0.11 new_mean_mag=13.8589 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:25:54.64 -21:47:12.9: 13.98 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.14
Forced photometry filter REJECTED candidate at 23:25:54.64 -21:47:12.9: ref_mag=14.00 +/- 0.14 new_mean_mag=13.8881 delta=0.12 (need > 0.90)
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:21:52.32 -21:42:40.0: 13.87 +/- 0.18 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.12
Forced photometry filter REJECTED candidate at 23:21:52.32 -21:42:40.0: ref_mag=13.92 +/- 0.12 new_mean_mag=13.8639 delta=0.06 (need > 0.90)
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:24:25.28 -20:17:24.4: 14.17 +/- 0.19 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:16:53.06 -21:22:36.8: 14.20 +/- 0.19 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:24:18.10 -22:08:58.3: 13.99 +/- 0.18 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:20:23.00 -21:30:08.3: 13.95 +/- 0.15 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:09:06.52 -21:59:55.0: 14.51 +/- 0.25 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:25:30.75 -21:33:35.4: 14.19 +/- 0.21 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:24:09.33 -21:22:26.0: 14.21 +/- 0.21 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:24:25.28 -20:17:24.4: 14.09 +/- 0.21 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:16:53.06 -21:22:36.8: 14.49 +/- 0.30 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.14
Forced photometry filter REJECTED candidate at 23:24:25.28 -20:17:24.4: ref_mag=14.13 +/- 0.14 new_mean_mag=13.9054 delta=0.23 (need > 0.90)
Forced photometry reference-image weighted average: 14.28 +/- 0.16
Forced photometry filter REJECTED candidate at 23:16:53.06 -21:22:36.8: ref_mag=14.28 +/- 0.16 new_mean_mag=13.8978 delta=0.39 (need > 0.90)
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:20:23.00 -21:30:08.3: 13.94 +/- 0.19 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:24:18.10 -22:08:58.3: 14.13 +/- 0.23 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:09:06.52 -21:59:55.0: 13.69 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.12
Forced photometry reference-image weighted average: 14.04 +/- 0.14
Forced photometry filter REJECTED candidate at 23:20:23.00 -21:30:08.3: ref_mag=13.94 +/- 0.12 new_mean_mag=13.8788 delta=0.07 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:24:18.10 -22:08:58.3: ref_mag=14.04 +/- 0.14 new_mean_mag=13.8072 delta=0.24 (need > 0.90)
Forced photometry reference-image weighted average: 13.90 +/- 0.13
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:25:30.75 -21:33:35.4: 14.04 +/- 0.21 detection
Forced photometry filter REJECTED candidate at 23:09:06.52 -21:59:55.0: ref_mag=13.90 +/- 0.13 new_mean_mag=13.8226 delta=0.08 (need > 0.90)
Forced photometry reference-image weighted average: 14.12 +/- 0.15
Forced photometry filter REJECTED candidate at 23:25:30.75 -21:33:35.4: ref_mag=14.12 +/- 0.15 new_mean_mag=13.9773 delta=0.14 (need > 0.90)
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:24:09.33 -21:22:26.0: 14.06 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.14 +/- 0.15
Forced photometry filter REJECTED candidate at 23:24:09.33 -21:22:26.0: ref_mag=14.14 +/- 0.15 new_mean_mag=14.0691 delta=0.07 (need > 0.90)
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:20:05.20 -21:40:16.4: 13.92 +/- 0.15 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:23:58.70 -20:39:06.4: 14.07 +/- 0.18 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:12:53.32 -22:09:27.8: 14.11 +/- 0.17 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:03:57.21 -20:39:47.2: 14.06 +/- 0.16 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:04:23.60 -17:16:33.6: 13.91 +/- 0.13 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:22:48.60 -21:53:21.7: 14.53 +/- 0.28 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:23:58.70 -20:39:06.4: 13.70 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.11
Forced photometry filter REJECTED candidate at 23:23:58.70 -20:39:06.4: ref_mag=13.85 +/- 0.11 new_mean_mag=13.9432 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:12:53.32 -22:09:27.8: 14.34 +/- 0.26 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:20:05.20 -21:40:16.4: 13.91 +/- 0.18 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:04:23.60 -17:16:33.6: 14.27 +/- 0.20 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:03:57.21 -20:39:47.2: 14.26 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.14
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:22:48.60 -21:53:21.7: 13.85 +/- 0.18 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.12
Forced photometry filter REJECTED candidate at 23:12:53.32 -22:09:27.8: ref_mag=14.18 +/- 0.14 new_mean_mag=13.9762 delta=0.20 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:20:05.20 -21:40:16.4: ref_mag=13.92 +/- 0.12 new_mean_mag=13.9659 delta=-0.05 (need > 0.90)
Forced photometry reference-image weighted average: 14.01 +/- 0.11
Forced photometry reference-image weighted average: 14.12 +/- 0.13
Forced photometry reference-image weighted average: 14.04 +/- 0.15
Forced photometry filter REJECTED candidate at 23:04:23.60 -17:16:33.6: ref_mag=14.01 +/- 0.11 new_mean_mag=14.0017 delta=0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:03:57.21 -20:39:47.2: ref_mag=14.12 +/- 0.13 new_mean_mag=14.0002 delta=0.12 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:22:48.60 -21:53:21.7: ref_mag=14.04 +/- 0.15 new_mean_mag=13.9434 delta=0.10 (need > 0.90)
Adding exclusion_list_local.txt__out21360.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22809.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 20751_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 20751_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 21100_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 21100_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
**** FOUND 23:04:00.60 -20:54:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21360_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
Preparing report for the candidate 21360_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
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Considering the candidate 21689_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
Preparing report for the candidate 21689_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
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Considering the candidate 22337_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 22337_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
**** FOUND 23:23:10.76 -20:08:36.1 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 22809_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
Preparing report for the candidate 22809_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
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Considering the candidate 22853_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 22853_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 23475_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 23475_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 23491_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 23491_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 23609_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 23609_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 23619_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 23619_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 23633_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 23633_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 23653_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 23653_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 23684_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 23684_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 23690_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 23690_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 23700_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 23700_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 23701_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 23701_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 23726_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 23726_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 23739_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 23739_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 23777_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 23777_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 23787_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 23787_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 23822_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 23822_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 23828_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 23828_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 23836_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 23836_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 23840_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 23840_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 23846_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 23846_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 23850_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 23850_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 23858_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 23858_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 23882_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 23882_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 23971_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 23971_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 24081_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 24081_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 24196_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 24196_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 04362_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 04362_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks
**** FOUND 22:57:06.60 -20:20:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 09035_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249
The candidate 09035_fd_Aqr-07-Q2b1x1_2026-10-11_23-45-09_20.00sec_0.00C_LIGHT_0249 did not pass the final checks