This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 07 26.4651 2461247.9651 10.96 21:54:22.60 -12:09:53.4
43.85379 -45.98107 galactic Cap Second-epoch detections are separated by 0.2" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.354 Eleonora -0 -0 0 10.8 -0 -0
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 21:54:22.60 -12:09:53.4: 15.22 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 21:54:22.60 -12:09:53.4: 15.85 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.4651* 21 54 22.60 -12 09 53.4 11.0 U Cap 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461247.9651,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260726.4651 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.4651 2461247.9651 11.49 22:26:31.42 -12:33:56.7
48.93016 -53.12344 galactic Aqr Second-epoch detections are separated by 1.0" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.100 Hekate -0 -1 1 11.6 0 0
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 22:26:31.42 -12:33:56.7: 15.27 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 22:26:31.42 -12:33:56.7: 15.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461247.9651,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260726.4651 11.49CV 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: 2461211.88265034 20.06.2026 09:10:50.989 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
First image: 2461211.88265034 20.06.2026 09:10:50.989 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
Last image: 2461247.96531854 26.07.2026 11:09:53.522 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.00
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: 6 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5325
Objects passed selection criteria: 5304
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 4030.5
Average stars matched: 3240.25 (80.3933 %)
Memory usage VmPeak: 232780 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jul 26 03:08:32 CDT 2026
VaST build number 1.0rc89-174-g9b7cb13a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-26)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jul 26 07:07:24 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: 2461211.88265034 20.06.2026 09:10:50.989 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
First image: 2461211.88265034 20.06.2026 09:10:50.989 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
Last image: 2461247.96531854 26.07.2026 11:09:53.522 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 16
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.72
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: 32 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 31472
Objects passed selection criteria: 31370
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 24456.5
Average stars matched: 21297.5 (87.0832 %)
Memory usage VmPeak: 257580 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jul 26 03:08:32 CDT 2026
VaST build number 1.0rc89-174-g9b7cb13a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-26)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jul 26 07:13:53 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
SExtractor catalog cache: saved Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.cat to cache
SExtractor catalog cache: saved Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461247.96481831
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits exists and is non-empty
Saving wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits to local_wcs_cache/
'wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits' -> 'local_wcs_cache/wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits'
wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits exists and is non-empty
Saving wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits to local_wcs_cache/
'wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits' -> 'local_wcs_cache/wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits'
wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits exists and is non-empty
Saving wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits to local_wcs_cache/
'wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits' -> 'local_wcs_cache/wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits'
wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits exists and is non-empty
Saving wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits to local_wcs_cache/
'wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits' -> 'local_wcs_cache/wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits (1st reference image)
verification OK: wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
Image size: 937.3'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:07.716 -09:59:55.69 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits (1st new image)
verification OK: wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
Image size: 941.4'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:16:55.698 -09:57:44.84 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:17:07.716 -09:59:55.69
Second-epoch image center 22:16:55.698 -09:57:44.84
Angular distance between the image centers 0.0613 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits (2nd new image)
verification OK: wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
Image size: 941.4'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:16:55.474 -09:57:29.78 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:17:07.716 -09:59:55.69
Second-epoch image center 22:16:55.474 -09:57:29.78
Angular distance between the image centers 0.0645 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 22:16:55.698 -09:57:44.84
Second-epoch second image center 22:16:55.474 -09:57:29.78
Angular distance between the image centers 0.00428 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-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits &> /tmp/tmp.OUKtXBYRGx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits &> /tmp/tmp.W2XpMtuWGz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits &> /tmp/tmp.4Nhk5UCZ6E
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits &> /tmp/tmp.HgU1GnWFDG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits and wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.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-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits and wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat
Found non-empty wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits and wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat
The reference image (wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits) and catalog (wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat) found
'wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat' -> 'wcsmag.cat'
Read 5318 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2566 to 342.3670 deg, Dec -15.2671 to -4.6696 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 326.2566 to 342.3670 deg, Dec -15.2671 to -4.6696 deg
Loaded 5068 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): 3783 out of 3855 total matches.
Matched with Tycho-2 3855 out of 5318 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.580000
a=0.000000 b=1.000000 c=22.580000
From vast_summary.log: estimated ref. image limiting mag.: -8.00
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.58
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.58
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5318 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2566 to 342.3670 deg, Dec -15.2671 to -4.6696 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 326.2566 to 342.3670 deg, Dec -15.2671 to -4.6696 deg
Loaded 5068 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): 3783 out of 3855 total matches.
Matched with Tycho-2 3855 out of 5318 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits -> calib.txt_param_ref_wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits (aperture=6.4)
Read 8439 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2518 to 342.4086 deg, Dec -15.2463 to -4.6697 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 326.2518 to 342.4086 deg, Dec -15.2463 to -4.6697 deg
Loaded 5075 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): 4285 out of 4418 total matches.
Matched with Tycho-2 4418 out of 8439 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits -> calib.txt_param_ref_wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits (aperture=6.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
2.4 pix Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
2.1 pix fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
2.1 pix fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
2.3 pix wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
2.4 pix wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
Limiting magnitude estimates:
14.6 mag. Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
15.2 mag. Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
13.3 mag. fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
13.3 mag. fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
All-image limiting magnitude estimate: 13.3 (SNR ) 10.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.OUKtXBYRGx (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits' -> 'wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.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-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
WCS-calibrated image found: wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
Checking if the catalog wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
WCS catalog name: wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=331, bad_region=0, passed=5318
Got 5318 stars (including 4983 good ones) from the SExtractor catalog wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat
util/solve_plate_with_UCAC5 got 5318 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 890 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 890 matched stars entering correct_measured_positions(), 880 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 890 matched stars entering correct_measured_positions(), 5253 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 890 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 890 matched stars entering correct_measured_positions(), 5249 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 890 matched stars entering correct_measured_positions(), 5249 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 890 stars left (next iteration limit 979)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits N_match=890 sigma_overall_arcsec=0.447 sigma_q1_arcsec=0.387 sigma_q2_arcsec=0.512 sigma_q3_arcsec=0.399 sigma_q4_arcsec=0.589 n_q1=245 n_q2=217 n_q3=218 n_q4=210 worst_quadrant_to_overall_ratio=1.317
The image catalog is written to wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits -region wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.W2XpMtuWGz (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits 856.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits' -> 'wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits'
This WCS solution (swarp) 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-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
WCS-calibrated image found: wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
Checking if the catalog wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
WCS catalog name: wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=484, bad_region=0, passed=8439
Got 8439 stars (including 7944 good ones) from the SExtractor catalog wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat
util/solve_plate_with_UCAC5 got 8439 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 901 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 894 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 8340 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 901 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 8341 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 8341 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 901 stars left (next iteration limit 991)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits (swarp) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits N_match=901 sigma_overall_arcsec=0.360 sigma_q1_arcsec=0.274 sigma_q2_arcsec=0.411 sigma_q3_arcsec=0.345 sigma_q4_arcsec=0.440 n_q1=245 n_q2=211 n_q3=225 n_q4=220 worst_quadrant_to_overall_ratio=1.222
The image catalog is written to wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits -region wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.4Nhk5UCZ6E (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
Checking if the catalog wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
WCS catalog name: wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=341, bad_region=0, passed=1253
Got 1253 stars (including 910 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat
util/solve_plate_with_UCAC5 got 1253 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.5 to -4.3)
Done reading UCAC5 zone files...
Matched 805 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 802 matched stars entering correct_measured_positions(), 784 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 802 matched stars entering correct_measured_positions(), 1216 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.5 to -4.3)
Done reading UCAC5 zone files...
Matched 805 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 802 matched stars entering correct_measured_positions(), 1215 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 802 matched stars entering correct_measured_positions(), 1215 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 802 stars left (next iteration limit 882)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=802 robust_rms=13.084 arcsec
SIP_REFIT: SIP order 3 trial: matched=802 robust_rms=0.515 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=802 robust_rms_before=0.965 arcsec robust_rms_before_corrected=0.371 arcsec robust_rms_after=0.515 arcsec
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best baseline 0.371 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits N_match=802 sigma_overall_arcsec=0.378 sigma_q1_arcsec=0.381 sigma_q2_arcsec=0.381 sigma_q3_arcsec=0.358 sigma_q4_arcsec=0.375 n_q1=176 n_q2=205 n_q3=199 n_q4=222 worst_quadrant_to_overall_ratio=1.008
The image catalog is written to wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits -region wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.HgU1GnWFDG (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
Checking if the catalog wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
WCS catalog name: wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=356, bad_region=0, passed=1192
Got 1192 stars (including 834 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits.wcscat
util/solve_plate_with_UCAC5 got 1192 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.5 to -4.3)
Done reading UCAC5 zone files...
Matched 741 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 738 matched stars entering correct_measured_positions(), 705 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 738 matched stars entering correct_measured_positions(), 1123 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.5 to -4.3)
Done reading UCAC5 zone files...
Matched 741 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 738 matched stars entering correct_measured_positions(), 1126 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 738 matched stars entering correct_measured_positions(), 1126 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 738 stars left (next iteration limit 811)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=738 robust_rms=13.362 arcsec
SIP_REFIT: SIP order 3 trial: matched=738 robust_rms=0.513 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=738 robust_rms_before=0.945 arcsec robust_rms_before_corrected=0.373 arcsec robust_rms_after=0.513 arcsec
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best baseline 0.373 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits N_match=738 sigma_overall_arcsec=0.383 sigma_q1_arcsec=0.405 sigma_q2_arcsec=0.361 sigma_q3_arcsec=0.357 sigma_q4_arcsec=0.420 n_q1=163 n_q2=193 n_q3=177 n_q4=205 worst_quadrant_to_overall_ratio=1.098
The image catalog is written to wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits -region wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits sigma_overall=0.447 worst_q_ratio=1.317
ref2=Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits sigma_overall=0.360 worst_q_ratio=1.222
new1=fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits sigma_overall=0.378 worst_q_ratio=1.008
new2=fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits sigma_overall=0.383 worst_q_ratio=1.098
reference average sigma_overall=0.4035 worst_q_ratio=1.2695
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1_astrometric_residuals.png (890 matched stars from wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2_astrometric_residuals.png (901 matched stars from wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444_astrometric_residuals.png (802 matched stars from wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445_astrometric_residuals.png (738 matched stars from wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits'
Saving fully-calibrated image wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits'
Preparing the HTML report for the field Aqr-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Aqr-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
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-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
SExtractor catalog cache: saved Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.cat to cache
SExtractor catalog cache: saved Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
Creating symlink local_wcs_cache/wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits exists and is non-empty
wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits exists and is non-empty
wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits exists and is non-empty
wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits (1st reference image)
verification OK: wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
Image size: 937.3'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:07.716 -09:59:55.69 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits (1st new image)
verification OK: wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
Image size: 941.4'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:16:55.698 -09:57:44.84 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:17:07.716 -09:59:55.69
Second-epoch image center 22:16:55.698 -09:57:44.84
Angular distance between the image centers 0.0613 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits (2nd new image)
verification OK: wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
Image size: 941.4'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:16:55.474 -09:57:29.78 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:17:07.716 -09:59:55.69
Second-epoch image center 22:16:55.474 -09:57:29.78
Angular distance between the image centers 0.0645 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 22:16:55.698 -09:57:44.84
Second-epoch second image center 22:16:55.474 -09:57:29.78
Angular distance between the image centers 0.00428 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-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits &> /tmp/tmp.wzsIcMgg76
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits &> /tmp/tmp.eJ34B7z5di
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits &> /tmp/tmp.fNAyy2l0Zq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits &> /tmp/tmp.ni9VKQYjTH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits and wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.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-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits and wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat
Found non-empty wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits and wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat
The reference image (wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits) and catalog (wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat) found
'wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat' -> 'wcsmag.cat'
Read 31665 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2518 to 342.4049 deg, Dec -15.2687 to -4.6696 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 326.2518 to 342.4049 deg, Dec -15.2687 to -4.6696 deg
Loaded 5086 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): 4178 out of 4455 total matches.
Matched with Tycho-2 4455 out of 31665 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.443700
a=0.000000 b=1.000000 c=22.443700
From vast_summary.log: estimated ref. image limiting mag.: -7.72
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.72
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.72
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 31665 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2518 to 342.4049 deg, Dec -15.2687 to -4.6696 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 326.2518 to 342.4049 deg, Dec -15.2687 to -4.6696 deg
Loaded 5086 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): 4178 out of 4455 total matches.
Matched with Tycho-2 4455 out of 31665 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits -> calib.txt_param_ref_wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits (aperture=5.0)
Read 43541 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2516 to 342.4086 deg, Dec -15.2553 to -4.6543 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 326.2516 to 342.4086 deg, Dec -15.2553 to -4.6543 deg
Loaded 5090 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): 4047 out of 4457 total matches.
Matched with Tycho-2 4457 out of 43541 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits -> calib.txt_param_ref_wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits (aperture=5.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 16 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
2.3 pix Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
1.8 pix fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
1.8 pix fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
2.2 pix wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
2.3 pix wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
Limiting magnitude estimates:
14.7 mag. Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
15.3 mag. Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
13.3 mag. fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
13.2 mag. fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 12.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.wzsIcMgg76 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits' -> 'wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.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-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
WCS-calibrated image found: wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
Checking if the catalog wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
WCS catalog name: wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=1237, bad_region=0, passed=31646
Got 31646 stars (including 30372 good ones) from the SExtractor catalog wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat
util/solve_plate_with_UCAC5 got 31646 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 880 matched stars entering correct_measured_positions(), 875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 880 matched stars entering correct_measured_positions(), 31229 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 880 matched stars entering correct_measured_positions(), 31229 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 880 matched stars entering correct_measured_positions(), 31229 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 880 stars left (next iteration limit 968)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits N_match=880 sigma_overall_arcsec=0.459 sigma_q1_arcsec=0.359 sigma_q2_arcsec=0.564 sigma_q3_arcsec=0.419 sigma_q4_arcsec=0.595 n_q1=248 n_q2=201 n_q3=221 n_q4=210 worst_quadrant_to_overall_ratio=1.298
The image catalog is written to wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits -region wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.eJ34B7z5di (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits 856.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits' -> 'wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits'
This WCS solution (swarp) 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-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
WCS-calibrated image found: wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
Checking if the catalog wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
WCS catalog name: wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=39, blended=2096, bad_region=0, passed=43502
Got 43502 stars (including 41351 good ones) from the SExtractor catalog wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat
util/solve_plate_with_UCAC5 got 43502 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 897 matched stars entering correct_measured_positions(), 891 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 897 matched stars entering correct_measured_positions(), 42954 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
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 897 matched stars entering correct_measured_positions(), 42954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 897 matched stars entering correct_measured_positions(), 42954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 897 stars left (next iteration limit 986)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits N_match=897 sigma_overall_arcsec=0.356 sigma_q1_arcsec=0.261 sigma_q2_arcsec=0.415 sigma_q3_arcsec=0.344 sigma_q4_arcsec=0.474 n_q1=246 n_q2=204 n_q3=231 n_q4=216 worst_quadrant_to_overall_ratio=1.334
The image catalog is written to wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits -region wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.fNAyy2l0Zq (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
Checking if the catalog wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
WCS catalog name: wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=576, bad_region=0, passed=12025
Got 12025 stars (including 11429 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat
util/solve_plate_with_UCAC5 got 12025 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 888 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 886 matched stars entering correct_measured_positions(), 873 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 886 matched stars entering correct_measured_positions(), 11812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 888 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 887 matched stars entering correct_measured_positions(), 11811 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 887 matched stars entering correct_measured_positions(), 11811 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 887 stars left (next iteration limit 974)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits N_match=887 sigma_overall_arcsec=0.418 sigma_q1_arcsec=0.395 sigma_q2_arcsec=0.443 sigma_q3_arcsec=0.389 sigma_q4_arcsec=0.376 n_q1=206 n_q2=243 n_q3=208 n_q4=230 worst_quadrant_to_overall_ratio=1.061
The image catalog is written to wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits -region wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ni9VKQYjTH (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
Checking if the catalog wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
WCS catalog name: wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=2, blended=422, bad_region=0, passed=11418
Got 11418 stars (including 10978 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits.wcscat
util/solve_plate_with_UCAC5 got 11418 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 895 matched stars entering correct_measured_positions(), 882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 895 matched stars entering correct_measured_positions(), 11189 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 896 matched stars entering correct_measured_positions(), 11193 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 895 matched stars entering correct_measured_positions(), 11193 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 895 stars left (next iteration limit 984)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits N_match=895 sigma_overall_arcsec=0.374 sigma_q1_arcsec=0.403 sigma_q2_arcsec=0.418 sigma_q3_arcsec=0.334 sigma_q4_arcsec=0.353 n_q1=201 n_q2=254 n_q3=204 n_q4=236 worst_quadrant_to_overall_ratio=1.119
The image catalog is written to wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits -region wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-10_20.00sec_-0.00C_LIGHTs_0444.fits
Saving fully-calibrated image wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Aqr-04-Q1b1x1_061909_TTUQ1b1x1_1708317_xfls2mXx/wcs_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445.fits
Preparing the HTML report for the field Aqr-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 21:54:22.60 -12:09:53.4: 15.22 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 22:41:53.85 -12:24:23.0: 11.09 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 21:54:59.80 -11:58:10.3: 10.58 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 22:26:31.42 -12:33:56.7: 15.27 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 22:44:23.26 -14:42:35.5: 11.31 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 22:37:00.38 -07:34:41.9: 10.93 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 22:43:17.00 -06:23:58.6: 12.62 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 22:26:02.73 -05:10:20.5: 12.73 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 21:54:22.60 -12:09:53.4: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 22:44:23.26 -14:42:35.5: 11.22 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 22:41:53.85 -12:24:23.0: 11.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.08 +/- 0.00
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 21:54:59.80 -11:58:10.3: 10.52 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.24 +/- 0.01
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 22:21:16.14 -14:59:01.7: 12.15 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 22:41:53.85 -12:24:23.0: ref_mag=11.08 +/- 0.00 new_mean_mag=11.4836 delta=-0.40 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:44:23.26 -14:42:35.5: ref_mag=11.24 +/- 0.01 new_mean_mag=11.1581 delta=0.08 (need > 0.90)
Forced photometry reference-image weighted average: 10.53 +/- 0.00
Forced photometry filter REJECTED candidate at 21:54:59.80 -11:58:10.3: ref_mag=10.53 +/- 0.00 new_mean_mag=10.9426 delta=-0.41 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 22:26:31.42 -12:33:56.7: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 22:26:02.73 -05:10:20.5: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.02
Forced photometry filter REJECTED candidate at 22:26:02.73 -05:10:20.5: ref_mag=12.70 +/- 0.02 new_mean_mag=12.7411 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 22:36:20.90 -05:10:33.8: 12.84 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 22:37:00.38 -07:34:41.9: 10.89 +/- 0.00 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 22:43:17.00 -06:23:58.6: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.02
Forced photometry filter REJECTED candidate at 22:43:17.00 -06:23:58.6: ref_mag=12.57 +/- 0.02 new_mean_mag=12.8162 delta=-0.25 (need > 0.90)
Forced photometry reference-image weighted average: 10.90 +/- 0.00
Forced photometry filter REJECTED candidate at 22:37:00.38 -07:34:41.9: ref_mag=10.90 +/- 0.00 new_mean_mag=11.1070 delta=-0.21 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 22:21:16.14 -14:59:01.7: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Forced photometry filter REJECTED candidate at 22:21:16.14 -14:59:01.7: ref_mag=12.14 +/- 0.01 new_mean_mag=12.2341 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 22:36:20.90 -05:10:33.8: 12.71 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.02
Forced photometry filter REJECTED candidate at 22:36:20.90 -05:10:33.8: ref_mag=12.74 +/- 0.02 new_mean_mag=13.0027 delta=-0.26 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 22:19:08.91 -07:18:14.8: 12.91 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 22:19:08.91 -07:18:14.8: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Forced photometry filter REJECTED candidate at 22:19:08.91 -07:18:14.8: ref_mag=12.88 +/- 0.02 new_mean_mag=13.0402 delta=-0.16 (need > 0.90)
Adding exclusion_list_local.txt__out62222.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62262.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
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: 5s
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Considering the candidate 62138_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445
The candidate 62138_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
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Considering the candidate 62221_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445
The candidate 62221_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
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Considering the candidate 62222_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445
Preparing report for the candidate 62222_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445
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Considering the candidate 62228_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445
The candidate 62228_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
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Considering the candidate 62231_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445
The candidate 62231_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
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Considering the candidate 62262_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445
Preparing report for the candidate 62262_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445
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Considering the candidate 62272_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445
The candidate 62272_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
**** FOUND 22:43:10.22 -06:58:30.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 62273_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445
The candidate 62273_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 62295_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445
The candidate 62295_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 62343_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445
The candidate 62343_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 62405_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445
The candidate 62405_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
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Considering the candidate 62494_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445
The candidate 62494_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
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Considering the candidate 62518_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445
The candidate 62518_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
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Considering the candidate 62545_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445
The candidate 62545_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
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Considering the candidate 62551_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445
The candidate 62551_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
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Considering the candidate 01862_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445
The candidate 01862_fd_Aqr-04-Q1b1x1_2026-07-26_06-09-53_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks