This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 08 25.2972 2461277.7972 12.91 20:05:52.36 -05:14:00.6
36.79441 -18.92962 galactic Aql Second-epoch detections are separated by 1.0" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.273 Atropos 0 -0 0 13.2 -0 0
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 20:05:52.36 -05:14:00.6: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 20:05:52.36 -05:14:00.6: 15.54 +/- 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,2461277.7972,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260825.2972 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.2972 2461277.7972 12.77 19:35:05.05 -05:18:40.2
33.14071 -12.11964 galactic Aql Second-epoch detections are separated by 1.8" and 8.1 pix
The object was found in VSX 3" PW Aql
Type: RRAB
# Max. Min./Amp. JD0 Period
12.831 V 14.151 V 2436399.46500 0.475062000000
The object was not found in astcheck.
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:35:05.05 -05:18:40.2: 13.85 +/- 0.07 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:35:05.05 -05:18:40.2: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.04
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
PW Aql,2461277.7972,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
PW Aql 20260825.2972 12.77CV 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: 2461203.88244201 12.06.2026 09:10:32.990 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
First image: 2461203.88244201 12.06.2026 09:10:32.990 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
Last image: 2461277.79754118 25.08.2026 07:08:17.558 /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.75
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 13693
Objects passed selection criteria: 13617
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 9014.5
Average stars matched: 8725.25 (96.7913 %)
Memory usage VmPeak: 240892 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Aug 24 15:05:05 CDT 2026
VaST build number 1.0rc89-195-gae6eb4b1
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Aug 25 02:20:21 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: 2461203.88244201 12.06.2026 09:10:32.990 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
First image: 2461203.88244201 12.06.2026 09:10:32.990 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
Last image: 2461277.79754118 25.08.2026 07:08:17.558 /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 60
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.41
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: 30 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 126470
Objects passed selection criteria: 126247
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: 94024.8
Average stars matched: 88837.8 (94.4834 %)
Memory usage VmPeak: 531240 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Aug 24 15:05:05 CDT 2026
VaST build number 1.0rc89-195-gae6eb4b1
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Aug 25 02:21:28 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
SExtractor catalog cache: saved Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.cat to cache
SExtractor catalog cache: saved Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.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/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.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: 2461277.79684008
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits exists and is non-empty
wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits exists and is non-empty
wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits exists and is non-empty
wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits (1st reference image)
verification OK: wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
Image size: 937.1'x624.0' 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: 19:42:53.275 -01:59:56.67 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_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits (1st new image)
verification OK: wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
Image size: 937.0'x624.0' 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: 19:42:52.025 -01:59:51.27 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:42:53.275 -01:59:56.67
Second-epoch image center 19:42:52.025 -01:59:51.27
Angular distance between the image centers 0.0054 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits (2nd new image)
verification OK: wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
Image size: 937.0'x624.0' 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: 19:42:54.534 -02:00:24.54 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:42:53.275 -01:59:56.67
Second-epoch image center 19:42:54.534 -02:00:24.54
Angular distance between the image centers 0.0094 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 19:42:52.025 -01:59:51.27
Second-epoch second image center 19:42:54.534 -02:00:24.54
Angular distance between the image centers 0.01395 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/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits &> /tmp/tmp.m9SS4CXAN3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits &> /tmp/tmp.WK9LGi80E1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits &> /tmp/tmp.RVgSfISSv3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits &> /tmp/tmp.i716oBGDoa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.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_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits and wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.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_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits and wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat
Found non-empty wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits and wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat
The reference image (wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits) and catalog (wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat) found
'wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat' -> 'wcsmag.cat'
Read 20227 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 287.8574 to 303.5971 deg, Dec -7.2599 to +3.2634 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 287.8574 to 303.5971 deg, Dec -7.2599 to 3.2634 deg
Loaded 10289 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): 8488 out of 8950 total matches.
Matched with Tycho-2 8950 out of 20227 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.706950
a=0.000000 b=1.000000 c=22.706950
From vast_summary.log: estimated ref. image limiting mag.: -7.75
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.96
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.96
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 20227 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 287.8574 to 303.5971 deg, Dec -7.2599 to +3.2634 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 287.8574 to 303.5971 deg, Dec -7.2599 to 3.2634 deg
Loaded 10289 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): 8488 out of 8950 total matches.
Matched with Tycho-2 8950 out of 20227 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
Forced-photometry filter: calibrated wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits -> calib.txt_param_ref_wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits (aperture=6.1)
Read 20355 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 287.8562 to 303.5949 deg, Dec -7.2521 to +3.2742 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 287.8562 to 303.5949 deg, Dec -7.2521 to 3.2742 deg
Loaded 10292 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): 8460 out of 8944 total matches.
Matched with Tycho-2 8944 out of 20355 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
Forced-photometry filter: calibrated wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits -> calib.txt_param_ref_wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits (aperture=6.0)
____ 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:
2.4 pix Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
2.3 pix Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
2.2 pix fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
2.2 pix fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
Limiting magnitude estimates:
15.0 mag. Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
15.0 mag. Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
13.6 mag. fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
13.6 mag. fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 10.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.m9SS4CXAN3 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits' -> 'wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.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/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
WCS_IMAGE_NAME=wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
WCS-calibrated image found: wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
Checking if the catalog wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat corresponding to the image wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits alredy exist and is non-empty...
Catalog wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat corresponding to the image wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
WCS catalog name: wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1243, bad_region=5559, passed=20227
Got 20227 stars (including 13746 good ones) from the SExtractor catalog wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat
util/solve_plate_with_UCAC5 got 20227 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 4896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 15889 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 15889 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 15889 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 4895 stars left (next iteration limit 5385)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits N_match=4895 sigma_overall_arcsec=0.462 sigma_q1_arcsec=0.391 sigma_q2_arcsec=0.579 sigma_q3_arcsec=0.436 sigma_q4_arcsec=0.552 n_q1=1710 n_q2=1061 n_q3=1253 n_q4=871 worst_quadrant_to_overall_ratio=1.253
The image catalog is written to wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits -region wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.WK9LGi80E1 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits' -> 'wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.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/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
WCS_IMAGE_NAME=wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
WCS-calibrated image found: wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
Checking if the catalog wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat corresponding to the image wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits alredy exist and is non-empty...
Catalog wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat corresponding to the image wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
WCS catalog name: wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1255, bad_region=5422, passed=20355
Got 20355 stars (including 13974 good ones) from the SExtractor catalog wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat
util/solve_plate_with_UCAC5 got 20355 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4900 matched stars entering correct_measured_positions(), 4900 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4900 matched stars entering correct_measured_positions(), 16095 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4900 matched stars entering correct_measured_positions(), 16095 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 4900 matched stars entering correct_measured_positions(), 16095 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 4900 stars left (next iteration limit 5390)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits N_match=4900 sigma_overall_arcsec=0.467 sigma_q1_arcsec=0.407 sigma_q2_arcsec=0.531 sigma_q3_arcsec=0.457 sigma_q4_arcsec=0.521 n_q1=1731 n_q2=1024 n_q3=1295 n_q4=850 worst_quadrant_to_overall_ratio=1.138
The image catalog is written to wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits -region wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.RVgSfISSv3 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
WCS_IMAGE_NAME=wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
WCS-calibrated image found: wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
Checking if the catalog wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits.wcscat corresponding to the image wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits.wcscat corresponding to the image wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
WCS catalog name: wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=343, bad_region=979, passed=4311
Got 4311 stars (including 3051 good ones) from the SExtractor catalog wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits.wcscat
util/solve_plate_with_UCAC5 got 4311 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 3014 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2989 matched stars entering correct_measured_positions(), 2989 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2989 matched stars entering correct_measured_positions(), 3544 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 3014 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2989 matched stars entering correct_measured_positions(), 3544 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 2989 matched stars entering correct_measured_positions(), 3544 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 2989 stars left (next iteration limit 3287)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2989 robust_rms=7.007 arcsec worst_quadrant_rms=8.498 arcsec
SIP_REFIT: SIP order 3 trial: matched=2989 robust_rms=0.503 arcsec worst_quadrant_rms=0.564 arcsec
SIP_REFIT: SIP order 5 trial: matched=2989 robust_rms=0.450 arcsec worst_quadrant_rms=0.538 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=2989 robust_rms_before=0.689 arcsec robust_rms_before_corrected=0.495 arcsec robust_rms_after=0.503 arcsec worst_quadrant_rms_before=0.606 worst_quadrant_rms_after=0.564
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.606 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits N_match=2989 sigma_overall_arcsec=0.500 sigma_q1_arcsec=0.448 sigma_q2_arcsec=0.598 sigma_q3_arcsec=0.480 sigma_q4_arcsec=0.543 n_q1=1049 n_q2=674 n_q3=740 n_q4=526 worst_quadrant_to_overall_ratio=1.197
The image catalog is written to wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits -region wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.i716oBGDoa (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
WCS_IMAGE_NAME=wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
WCS-calibrated image found: wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
Checking if the catalog wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits.wcscat corresponding to the image wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits.wcscat corresponding to the image wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
WCS catalog name: wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=351, bad_region=974, passed=4349
Got 4349 stars (including 3089 good ones) from the SExtractor catalog wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits.wcscat
util/solve_plate_with_UCAC5 got 4349 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.2)
Done reading UCAC5 zone files...
Matched 3057 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3031 matched stars entering correct_measured_positions(), 3031 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3031 matched stars entering correct_measured_positions(), 3574 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.2)
Done reading UCAC5 zone files...
Matched 3058 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3031 matched stars entering correct_measured_positions(), 3574 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 3031 matched stars entering correct_measured_positions(), 3574 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 3031 stars left (next iteration limit 3334)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3031 robust_rms=7.070 arcsec worst_quadrant_rms=8.660 arcsec
SIP_REFIT: SIP order 3 trial: matched=3031 robust_rms=0.503 arcsec worst_quadrant_rms=0.540 arcsec
SIP_REFIT: SIP order 5 trial: matched=3031 robust_rms=0.443 arcsec worst_quadrant_rms=0.527 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=3031 robust_rms_before=0.681 arcsec robust_rms_before_corrected=0.470 arcsec robust_rms_after=0.503 arcsec worst_quadrant_rms_before=0.550 worst_quadrant_rms_after=0.540
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.550 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits N_match=3031 sigma_overall_arcsec=0.480 sigma_q1_arcsec=0.412 sigma_q2_arcsec=0.555 sigma_q3_arcsec=0.481 sigma_q4_arcsec=0.502 n_q1=1074 n_q2=678 n_q3=754 n_q4=525 worst_quadrant_to_overall_ratio=1.158
The image catalog is written to wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits -region wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits to local_wcs_cache/
'wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits' -> 'local_wcs_cache/wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits'
Saving the final (post-refit) wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits to local_wcs_cache/
'wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits' -> 'local_wcs_cache/wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits'
Saving the final (post-refit) wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits to local_wcs_cache/
'wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits' -> 'local_wcs_cache/wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits'
Saving the final (post-refit) wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits to local_wcs_cache/
'wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits' -> 'local_wcs_cache/wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits sigma_overall=0.462 worst_q_ratio=1.253
ref2=Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits sigma_overall=0.467 worst_q_ratio=1.138
new1=fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits sigma_overall=0.500 worst_q_ratio=1.197
new2=fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits sigma_overall=0.480 worst_q_ratio=1.158
reference average sigma_overall=0.4645 worst_q_ratio=1.1955
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226_astrometric_residuals.png (4895 matched stars from wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.42 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290_astrometric_residuals.png (4900 matched stars from wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181_astrometric_residuals.png (2989 matched stars from wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.44 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182_astrometric_residuals.png (3031 matched stars from wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.41 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits'
Saving fully-calibrated image wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits'
Preparing the HTML report for the field Aql-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Aql-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
SExtractor catalog cache: saved Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.cat to cache
SExtractor catalog cache: saved Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
Creating symlink local_wcs_cache/wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits exists and is non-empty
wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits exists and is non-empty
wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits exists and is non-empty
wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits (1st reference image)
verification OK: wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
Image size: 937.1'x624.0' 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: 19:42:53.275 -01:59:56.67 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_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits (1st new image)
verification OK: wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
Image size: 937.0'x624.0' 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: 19:42:52.025 -01:59:51.27 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:42:53.275 -01:59:56.67
Second-epoch image center 19:42:52.025 -01:59:51.27
Angular distance between the image centers 0.0054 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits (2nd new image)
verification OK: wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
Image size: 937.0'x624.0' 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: 19:42:54.534 -02:00:24.54 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:42:53.275 -01:59:56.67
Second-epoch image center 19:42:54.534 -02:00:24.54
Angular distance between the image centers 0.0094 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 19:42:52.025 -01:59:51.27
Second-epoch second image center 19:42:54.534 -02:00:24.54
Angular distance between the image centers 0.01395 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/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits &> /tmp/tmp.4mkClPLM4N
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits &> /tmp/tmp.g74yk4VpOi
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits &> /tmp/tmp.up5HnkayTh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits &> /tmp/tmp.lt6Jrg8Qnu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.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_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits and wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.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_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits and wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat
Found non-empty wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits and wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat
The reference image (wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits) and catalog (wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat) found
'wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat' -> 'wcsmag.cat'
Read 167162 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 287.8558 to 303.5989 deg, Dec -7.2624 to +3.2650 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 287.8558 to 303.5989 deg, Dec -7.2624 to 3.2650 deg
Loaded 10296 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): 7300 out of 9230 total matches.
Matched with Tycho-2 9230 out of 167162 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.545200
a=0.000000 b=1.000000 c=22.545200
From vast_summary.log: estimated ref. image limiting mag.: -7.41
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.14
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.14
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 167162 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 287.8558 to 303.5989 deg, Dec -7.2624 to +3.2650 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 287.8558 to 303.5989 deg, Dec -7.2624 to 3.2650 deg
Loaded 10296 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): 7300 out of 9230 total matches.
Matched with Tycho-2 9230 out of 167162 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
Forced-photometry filter: calibrated wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits -> calib.txt_param_ref_wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits (aperture=4.7)
Read 183128 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 287.8553 to 303.5977 deg, Dec -7.2536 to +3.2758 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 287.8553 to 303.5977 deg, Dec -7.2536 to 3.2758 deg
Loaded 10297 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): 7125 out of 9225 total matches.
Matched with Tycho-2 9225 out of 183128 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
Forced-photometry filter: calibrated wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits -> calib.txt_param_ref_wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 44 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
2.1 pix Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
2.0 pix fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
2.0 pix fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
Limiting magnitude estimates:
15.1 mag. Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
15.2 mag. Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
13.8 mag. fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
13.8 mag. fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 13.3 (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.4mkClPLM4N (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits' -> 'wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.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/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
WCS_IMAGE_NAME=wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
WCS-calibrated image found: wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
Checking if the catalog wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat corresponding to the image wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits alredy exist and is non-empty...
Catalog wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat corresponding to the image wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
WCS catalog name: wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=19123, bad_region=31897, passed=167147
Got 167147 stars (including 120817 good ones) from the SExtractor catalog wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat
util/solve_plate_with_UCAC5 got 167147 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 4912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 143311 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 143311 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 143313 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 4912 stars left (next iteration limit 5403)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits N_match=4912 sigma_overall_arcsec=0.454 sigma_q1_arcsec=0.384 sigma_q2_arcsec=0.547 sigma_q3_arcsec=0.433 sigma_q4_arcsec=0.538 n_q1=1725 n_q2=1034 n_q3=1334 n_q4=819 worst_quadrant_to_overall_ratio=1.205
The image catalog is written to wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits -region wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.g74yk4VpOi (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits' -> 'wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.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/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
WCS_IMAGE_NAME=wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
WCS-calibrated image found: wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
Checking if the catalog wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat corresponding to the image wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits alredy exist and is non-empty...
Catalog wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat corresponding to the image wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
WCS catalog name: wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=21567, bad_region=35769, passed=183109
Got 183109 stars (including 130765 good ones) from the SExtractor catalog wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat
util/solve_plate_with_UCAC5 got 183109 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4915 matched stars entering correct_measured_positions(), 4915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4915 matched stars entering correct_measured_positions(), 156363 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4916 matched stars entering correct_measured_positions(), 156363 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 4916 matched stars entering correct_measured_positions(), 156363 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 4916 stars left (next iteration limit 5406)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits N_match=4916 sigma_overall_arcsec=0.443 sigma_q1_arcsec=0.399 sigma_q2_arcsec=0.510 sigma_q3_arcsec=0.423 sigma_q4_arcsec=0.501 n_q1=1717 n_q2=991 n_q3=1376 n_q4=832 worst_quadrant_to_overall_ratio=1.150
The image catalog is written to wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits -region wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.up5HnkayTh (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
WCS_IMAGE_NAME=wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
WCS-calibrated image found: wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
Checking if the catalog wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits.wcscat corresponding to the image wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits.wcscat corresponding to the image wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
WCS catalog name: wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=2342, bad_region=8240, passed=55729
Got 55729 stars (including 45742 good ones) from the SExtractor catalog wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits.wcscat
util/solve_plate_with_UCAC5 got 55729 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4908 matched stars entering correct_measured_positions(), 4908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4908 matched stars entering correct_measured_positions(), 49838 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4909 matched stars entering correct_measured_positions(), 49838 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 4909 matched stars entering correct_measured_positions(), 49838 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 4909 stars left (next iteration limit 5398)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4909 robust_rms=6.670 arcsec worst_quadrant_rms=8.203 arcsec
SIP_REFIT: SIP order 3 trial: matched=4909 robust_rms=0.495 arcsec worst_quadrant_rms=0.531 arcsec
SIP_REFIT: SIP order 5 trial: matched=4909 robust_rms=0.445 arcsec worst_quadrant_rms=0.506 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=4909 robust_rms_before=0.682 arcsec robust_rms_before_corrected=0.464 arcsec robust_rms_after=0.495 arcsec worst_quadrant_rms_before=0.541 worst_quadrant_rms_after=0.531
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.541 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits N_match=4909 sigma_overall_arcsec=0.475 sigma_q1_arcsec=0.430 sigma_q2_arcsec=0.549 sigma_q3_arcsec=0.457 sigma_q4_arcsec=0.532 n_q1=1814 n_q2=1007 n_q3=1311 n_q4=777 worst_quadrant_to_overall_ratio=1.157
The image catalog is written to wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits -region wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.lt6Jrg8Qnu (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
WCS_IMAGE_NAME=wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
WCS-calibrated image found: wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
Checking if the catalog wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits.wcscat corresponding to the image wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits.wcscat corresponding to the image wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
WCS catalog name: wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=2378, bad_region=8145, passed=56168
Got 56168 stars (including 46204 good ones) from the SExtractor catalog wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits.wcscat
util/solve_plate_with_UCAC5 got 56168 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4905 matched stars entering correct_measured_positions(), 4905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4905 matched stars entering correct_measured_positions(), 50309 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 50309 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 50309 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 4906 stars left (next iteration limit 5395)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4906 robust_rms=6.663 arcsec worst_quadrant_rms=8.310 arcsec
SIP_REFIT: SIP order 3 trial: matched=4906 robust_rms=0.491 arcsec worst_quadrant_rms=0.521 arcsec
SIP_REFIT: SIP order 5 trial: matched=4906 robust_rms=0.432 arcsec worst_quadrant_rms=0.509 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=4906 robust_rms_before=0.676 arcsec robust_rms_before_corrected=0.445 arcsec robust_rms_after=0.491 arcsec worst_quadrant_rms_before=0.523 worst_quadrant_rms_after=0.521
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.523 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits N_match=4906 sigma_overall_arcsec=0.461 sigma_q1_arcsec=0.410 sigma_q2_arcsec=0.541 sigma_q3_arcsec=0.462 sigma_q4_arcsec=0.484 n_q1=1832 n_q2=1004 n_q3=1313 n_q4=757 worst_quadrant_to_overall_ratio=1.175
The image catalog is written to wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits -region wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-07-16_20.00sec_-0.00C_LIGHT_0181.fits
Saving fully-calibrated image wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Aql-04-Q2b1x1_021640_TTUQ2b1x1_242126_rlNvyqpu/wcs_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182.fits
Preparing the HTML report for the field Aql-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:48:37.04 +00:17:00.7: 12.96 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:41:51.23 -01:54:09.8: 12.95 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:52:14.10 -02:38:53.0: 13.71 +/- 0.07 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:42:31.98 -00:00:38.1: 12.92 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:50:40.17 +01:40:16.5: 12.68 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:46:56.06 -03:01:39.0: 12.62 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:42:34.51 -01:46:49.6: 12.81 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:47:38.82 +01:04:21.4: 12.58 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:52:23.90 -05:20:42.9: 12.76 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:46:56.06 -03:01:39.0: 12.67 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:50:40.17 +01:40:16.5: 12.72 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:42:31.98 -00:00:38.1: 13.01 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:42:34.51 -01:46:49.6: 12.88 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:48:37.04 +00:17:00.7: 12.93 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:41:51.23 -01:54:09.8: 12.96 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:52:14.10 -02:38:53.0: 13.67 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Forced photometry reference-image weighted average: 12.70 +/- 0.02
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Forced photometry filter REJECTED candidate at 19:46:56.06 -03:01:39.0: ref_mag=12.64 +/- 0.01 new_mean_mag=13.2990 delta=-0.65 (need > 0.90)
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Forced photometry reference-image weighted average: 13.69 +/- 0.05
Forced photometry filter REJECTED candidate at 19:50:40.17 +01:40:16.5: ref_mag=12.70 +/- 0.02 new_mean_mag=12.9739 delta=-0.27 (need > 0.90)
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Forced photometry filter REJECTED candidate at 19:42:34.51 -01:46:49.6: ref_mag=12.85 +/- 0.02 new_mean_mag=12.9962 delta=-0.15 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:42:31.98 -00:00:38.1: ref_mag=12.96 +/- 0.02 new_mean_mag=13.2551 delta=-0.29 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:48:37.04 +00:17:00.7: ref_mag=12.95 +/- 0.02 new_mean_mag=13.0615 delta=-0.12 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:41:51.23 -01:54:09.8: ref_mag=12.95 +/- 0.02 new_mean_mag=13.0616 delta=-0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:52:14.10 -02:38:53.0: ref_mag=13.69 +/- 0.05 new_mean_mag=13.5865 delta=0.10 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:47:38.82 +01:04:21.4: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.02
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:52:23.90 -05:20:42.9: 12.82 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 19:47:38.82 +01:04:21.4: ref_mag=12.59 +/- 0.02 new_mean_mag=12.7231 delta=-0.13 (need > 0.90)
Forced photometry reference-image weighted average: 12.79 +/- 0.02
Forced photometry filter REJECTED candidate at 19:52:23.90 -05:20:42.9: ref_mag=12.79 +/- 0.02 new_mean_mag=13.0311 delta=-0.24 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 20:05:52.36 -05:14:00.6: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:49:47.85 -02:02:46.7: 13.30 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:53:11.80 +00:20:36.4: 13.02 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:57:34.83 -01:51:21.3: 12.86 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:39:01.27 -00:52:42.0: 13.49 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:47:24.20 -03:26:58.7: 13.30 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 20:05:52.36 -05:14:00.6: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:39:11.20 -00:30:07.0: 13.34 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:41:27.39 -03:00:31.1: 13.52 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 20:04:38.91 +01:09:22.2: 13.22 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:49:47.85 -02:02:46.7: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:53:11.80 +00:20:36.4: 13.02 +/- 0.04 detection
Forced photometry filter REJECTED candidate at 19:49:47.85 -02:02:46.7: ref_mag=13.30 +/- 0.03 new_mean_mag=13.4267 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:57:34.83 -01:51:21.3: 12.86 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.03
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:39:01.27 -00:52:42.0: 13.64 +/- 0.05 detection
Forced photometry filter REJECTED candidate at 19:53:11.80 +00:20:36.4: ref_mag=13.02 +/- 0.03 new_mean_mag=13.1096 delta=-0.09 (need > 0.90)
Forced photometry reference-image weighted average: 12.86 +/- 0.02
Forced photometry filter REJECTED candidate at 19:57:34.83 -01:51:21.3: ref_mag=12.86 +/- 0.02 new_mean_mag=12.9503 delta=-0.09 (need > 0.90)
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Forced photometry filter REJECTED candidate at 19:39:01.27 -00:52:42.0: ref_mag=13.56 +/- 0.03 new_mean_mag=13.4463 delta=0.11 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:47:24.20 -03:26:58.7: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Forced photometry filter REJECTED candidate at 19:47:24.20 -03:26:58.7: ref_mag=13.30 +/- 0.03 new_mean_mag=13.4452 delta=-0.14 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:39:11.20 -00:30:07.0: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.03
Forced photometry filter REJECTED candidate at 19:39:11.20 -00:30:07.0: ref_mag=13.34 +/- 0.03 new_mean_mag=13.3130 delta=0.03 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:41:27.39 -03:00:31.1: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Forced photometry filter REJECTED candidate at 19:41:27.39 -03:00:31.1: ref_mag=13.49 +/- 0.03 new_mean_mag=13.4679 delta=0.02 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 20:04:38.91 +01:09:22.2: 13.11 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.03
Forced photometry filter REJECTED candidate at 20:04:38.91 +01:09:22.2: ref_mag=13.16 +/- 0.03 new_mean_mag=13.4895 delta=-0.32 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:35:05.05 -05:18:40.2: 13.85 +/- 0.07 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:35:05.05 -05:18:40.2: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.04
Forced photometry filter KEPT candidate at 19:35:05.05 -05:18:40.2: ref_mag=13.71 +/- 0.04 new_mean_mag=12.7652 delta=0.95 (need > 0.90)
Adding exclusion_list_local.txt__out131583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197759.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 71s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 197679_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197679_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
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Considering the candidate 197687_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197687_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 19:46:28.92 -01:31:52.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197695_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197695_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
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Considering the candidate 197696_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197696_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
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Considering the candidate 197700_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197700_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
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Considering the candidate 197702_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197702_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
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Considering the candidate 197703_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197703_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
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Considering the candidate 197707_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197707_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
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Considering the candidate 197708_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197708_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 19:59:03.09 +01:36:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197709_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197709_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 19:37:10.22 +00:16:42.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197711_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197711_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
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Considering the candidate 197717_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197717_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
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Considering the candidate 197723_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197723_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 19:29:09.86 +01:57:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197726_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197726_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 19:53:01.92 -03:38:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197741_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197741_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 19:37:53.40 -04:38:55.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 197746_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197746_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 19:58:31.29 -03:34:50.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197749_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197749_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 20:06:11.21 -04:06:00.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 197750_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197750_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 19:25:07.29 -04:52:44.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 197752_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197752_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 19:40:38.65 -00:38:10.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 197755_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197755_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 19:40:19.20 -05:25:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197756_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197756_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 19:43:27.40 +01:13:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197759_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
Preparing report for the candidate 197759_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
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Considering the candidate 197762_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197762_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 19:40:48.14 -00:36:49.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 197764_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197764_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 19:59:21.45 +01:20:52.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 197766_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197766_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 197767_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197767_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
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Considering the candidate 197768_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197768_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 20:01:34.45 -00:11:47.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197769_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197769_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 19:45:50.92 -02:51:22.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 197773_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197773_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
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Considering the candidate 197780_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197780_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
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Considering the candidate 197784_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197784_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
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Considering the candidate 197785_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197785_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
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Considering the candidate 197787_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197787_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
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Considering the candidate 197791_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197791_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 19:45:26.54 +01:25:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197792_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197792_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
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Considering the candidate 197794_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 197794_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
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Considering the candidate 184647_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 184647_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 20:00:08.90 -02:13:28.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 185250_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 185250_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 19:35:42.69 -00:11:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91952_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 91952_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 19:35:29.20 -01:44:18.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181948_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 181948_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 20:03:20.18 -01:29:32.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181840_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 181840_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 19:26:09.24 -02:30:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180696_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 180696_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks
**** FOUND 19:46:54.78 +02:13:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180603_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182
The candidate 180603_fd_Aql-04-Q2b1x1_2026-08-25_02-08-17_20.00sec_0.00C_LIGHT_0182 did not pass the final checks