This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 07 23.4495 2461244.9495 13.68 22:24:06.33 -10:04:22.5
51.97002 -51.36190 galactic Aqr Second-epoch detections are separated by 1.3" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.736 Harvard -0 0 0 13.5 0 0
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:24:06.33 -10:04:22.5: 15.38 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits at 22:24:06.33 -10:04:22.5: 15.38 +/- 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,2461244.9495,13.68,0.05,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 20260723.4495 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 23.4495 2461244.9495 13.94 22:13:30.65 -09:07:03.6
51.13639 -48.63318 galactic Aqr Second-epoch detections are separated by 0.1" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.2121 Sevastopol -0 1 1 14.2 -0 -0
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:13:30.65 -09:07:03.6: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits at 22:13:30.65 -09:07:03.6: 15.43 +/- 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,2461244.9495,13.94,0.05,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 20260723.4495 13.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 23.4495 2461244.9495 11.91 22:27:48.81 -07:29:01.9
56.21990 -50.72546 galactic Aqr Second-epoch detections are separated by 0.1" and 3.3 pix
The object was found in VSX 1" BN Aqr
Type: RRAB
# Max. Min./Amp. JD0 Period
11.770 V 12.940 V 2452900.64400 0.469682200000 F3
The object was not found in astcheck.
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:27:48.81 -07:29:01.9: 12.89 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits at 22:27:48.81 -07:29:01.9: 12.90 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.03
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
BN Aqr,2461244.9495,11.91,0.05,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
BN Aqr 20260723.4495 11.91CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461211.88265034 20.06.2026 09:10:50.989 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
First image: 2461211.88265034 20.06.2026 09:10:50.989 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
Last image: 2461244.94973057 23.07.2026 10:47:26.721 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.96
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: 13 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 4991
Objects passed selection criteria: 4979
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 3931.75
Average stars matched: 3597.75 (91.5051 %)
Memory usage VmPeak: 114264 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 22 16:05:55 CDT 2026
VaST build number 1.0rc89-166-g55a66cb7
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-22)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jul 23 06:58:41 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461211.88265034 20.06.2026 09:10:50.989 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
First image: 2461211.88265034 20.06.2026 09:10:50.989 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
Last image: 2461244.94973057 23.07.2026 10:47:26.721 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 76
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.65
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: 31 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 31023
Objects passed selection criteria: 30912
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 24613.5
Average stars matched: 22421.2 (91.0933 %)
Memory usage VmPeak: 133724 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 22 16:05:55 CDT 2026
VaST build number 1.0rc89-166-g55a66cb7
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-22)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jul 23 07:01:59 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
SExtractor catalog cache: saved Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.cat to cache
SExtractor catalog cache: saved Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.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: 2461244.94929865
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits exists and is non-empty
Saving wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits to local_wcs_cache/
'wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits' -> 'local_wcs_cache/wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits'
wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits exists and is non-empty
Saving wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits to local_wcs_cache/
'wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits' -> 'local_wcs_cache/wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits'
wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits exists and is non-empty
Saving wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits to local_wcs_cache/
'wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits' -> 'local_wcs_cache/wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits'
wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits exists and is non-empty
Saving wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits to local_wcs_cache/
'wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits' -> 'local_wcs_cache/wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits (1st reference image)
verification OK: wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
Image size: 937.3'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:07.716 -09:59:55.69 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits (1st new image)
verification OK: wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
Image size: 937.1'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:08.171 -10:00:10.68 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:17:07.716 -09:59:55.69
Second-epoch image center 22:17:08.171 -10:00:10.68
Angular distance between the image centers 0.0046 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits (2nd new image)
verification OK: wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
Image size: 937.2'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:08.981 -09:59:55.26 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:17:07.716 -09:59:55.69
Second-epoch image center 22:17:08.981 -09:59:55.26
Angular distance between the image centers 0.0052 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 22:17:08.171 -10:00:10.68
Second-epoch second image center 22:17:08.981 -09:59:55.26
Angular distance between the image centers 0.00542 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits &> /tmp/tmp.nMSojLOSbE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits &> /tmp/tmp.cJpNHeQDZ2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits &> /tmp/tmp.L5O1QyMObf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits &> /tmp/tmp.qSq5VsPLWr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits and wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits and wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat
Found non-empty wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits and wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat
The reference image (wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits) and catalog (wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat) found
'wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat' -> 'wcsmag.cat'
Read 5318 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2566 to 342.3670 deg, Dec -15.2671 to -4.6696 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 326.2566 to 342.3670 deg, Dec -15.2671 to -4.6696 deg
Loaded 5068 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3783 out of 3855 total matches.
Matched with Tycho-2 3855 out of 5318 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.567300
a=0.000000 b=1.000000 c=22.567300
From vast_summary.log: estimated ref. image limiting mag.: -7.96
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.61
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.61
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5318 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2566 to 342.3670 deg, Dec -15.2671 to -4.6696 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 326.2566 to 342.3670 deg, Dec -15.2671 to -4.6696 deg
Loaded 5068 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3783 out of 3855 total matches.
Matched with Tycho-2 3855 out of 5318 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits -> calib.txt_param_ref_wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits (aperture=6.2)
Read 5332 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2518 to 342.4085 deg, Dec -15.2464 to -4.6697 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 326.2518 to 342.4085 deg, Dec -15.2464 to -4.6697 deg
Loaded 5076 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): 3787 out of 3866 total matches.
Matched with Tycho-2 3866 out of 5332 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits -> calib.txt_param_ref_wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
2.3 pix Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits
2.3 pix fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
2.4 pix fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
2.3 pix wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
2.3 pix wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits
Limiting magnitude estimates:
14.6 mag. Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
14.6 mag. Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits
14.5 mag. fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
14.4 mag. fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.6 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.nMSojLOSbE (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_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits' -> 'wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
WCS-calibrated image found: wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
Checking if the catalog wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
WCS catalog name: wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=331, bad_region=1173, passed=5318
Got 5318 stars (including 3871 good ones) from the SExtractor catalog wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat
util/solve_plate_with_UCAC5 got 5318 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 882 matched stars entering correct_measured_positions(), 881 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 882 matched stars entering correct_measured_positions(), 4256 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 882 matched stars entering correct_measured_positions(), 4254 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 882 matched stars entering correct_measured_positions(), 4254 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 882 stars left (next iteration limit 970)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits N_match=882 sigma_overall_arcsec=0.383 sigma_q1_arcsec=0.390 sigma_q2_arcsec=0.356 sigma_q3_arcsec=0.386 sigma_q4_arcsec=0.423 n_q1=315 n_q2=147 n_q3=286 n_q4=134 worst_quadrant_to_overall_ratio=1.105
The image catalog is written to wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits -region wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.cJpNHeQDZ2 (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_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits' -> 'wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits
WCS-calibrated image found: wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits
Checking if the catalog wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits
WCS catalog name: wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.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=328, bad_region=1178, passed=5332
Got 5332 stars (including 3884 good ones) from the SExtractor catalog wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits.wcscat
util/solve_plate_with_UCAC5 got 5332 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 883 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 883 matched stars entering correct_measured_positions(), 881 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 883 matched stars entering correct_measured_positions(), 4289 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 883 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 883 matched stars entering correct_measured_positions(), 4288 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 883 matched stars entering correct_measured_positions(), 4288 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 883 stars left (next iteration limit 971)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits N_match=883 sigma_overall_arcsec=0.363 sigma_q1_arcsec=0.317 sigma_q2_arcsec=0.382 sigma_q3_arcsec=0.369 sigma_q4_arcsec=0.380 n_q1=315 n_q2=145 n_q3=286 n_q4=137 worst_quadrant_to_overall_ratio=1.051
The image catalog is written to wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits -region wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.L5O1QyMObf (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
Checking if the catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
WCS catalog name: wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.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=349, bad_region=1149, passed=4916
Got 4916 stars (including 3493 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits.wcscat
util/solve_plate_with_UCAC5 got 4916 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
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 889 matched stars entering correct_measured_positions(), 884 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 889 matched stars entering correct_measured_positions(), 3855 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 889 matched stars entering correct_measured_positions(), 3857 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 889 matched stars entering correct_measured_positions(), 3857 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 889 stars left (next iteration limit 977)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits N_match=889 sigma_overall_arcsec=0.363 sigma_q1_arcsec=0.327 sigma_q2_arcsec=0.372 sigma_q3_arcsec=0.351 sigma_q4_arcsec=0.302 n_q1=264 n_q2=183 n_q3=247 n_q4=195 worst_quadrant_to_overall_ratio=1.025
The image catalog is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits -region wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.qSq5VsPLWr (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
Checking if the catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
WCS catalog name: wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.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=304, bad_region=1116, passed=4867
Got 4867 stars (including 3492 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits.wcscat
util/solve_plate_with_UCAC5 got 4867 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 889 matched stars entering correct_measured_positions(), 887 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 889 matched stars entering correct_measured_positions(), 3844 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 889 matched stars entering correct_measured_positions(), 3843 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 889 matched stars entering correct_measured_positions(), 3843 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 889 stars left (next iteration limit 977)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits N_match=889 sigma_overall_arcsec=0.340 sigma_q1_arcsec=0.328 sigma_q2_arcsec=0.398 sigma_q3_arcsec=0.328 sigma_q4_arcsec=0.308 n_q1=260 n_q2=185 n_q3=250 n_q4=194 worst_quadrant_to_overall_ratio=1.169
The image catalog is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits -region wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits sigma_overall=0.383 worst_q_ratio=1.105
ref2=Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits sigma_overall=0.363 worst_q_ratio=1.051
new1=fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits sigma_overall=0.363 worst_q_ratio=1.025
new2=fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits sigma_overall=0.340 worst_q_ratio=1.169
reference average sigma_overall=0.373 worst_q_ratio=1.078
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_astrometric_residuals.png (882 matched stars from wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_astrometric_residuals.png (883 matched stars from wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476_astrometric_residuals.png (889 matched stars from wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477_astrometric_residuals.png (889 matched stars from wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits'
Saving fully-calibrated image wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits'
Preparing the HTML report for the field Aqr-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Aqr-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/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
SExtractor catalog cache: saved Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.cat to cache
SExtractor catalog cache: saved Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
Creating symlink local_wcs_cache/wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits exists and is non-empty
wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits exists and is non-empty
wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits exists and is non-empty
wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits (1st reference image)
verification OK: wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
Image size: 937.3'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:07.716 -09:59:55.69 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits (1st new image)
verification OK: wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
Image size: 937.1'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:08.171 -10:00:10.68 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:17:07.716 -09:59:55.69
Second-epoch image center 22:17:08.171 -10:00:10.68
Angular distance between the image centers 0.0046 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits (2nd new image)
verification OK: wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
Image size: 937.2'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:08.981 -09:59:55.26 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:17:07.716 -09:59:55.69
Second-epoch image center 22:17:08.981 -09:59:55.26
Angular distance between the image centers 0.0052 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 22:17:08.171 -10:00:10.68
Second-epoch second image center 22:17:08.981 -09:59:55.26
Angular distance between the image centers 0.00542 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits &> /tmp/tmp.ac2Fs0LXJW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits &> /tmp/tmp.l4rU3unTJ5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits &> /tmp/tmp.ApvZJWoExo
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits &> /tmp/tmp.71QpEvyUD3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits and wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits and wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat
Found non-empty wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits and wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat
The reference image (wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits) and catalog (wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat) found
'wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat' -> 'wcsmag.cat'
Read 31665 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2518 to 342.4049 deg, Dec -15.2687 to -4.6696 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 326.2518 to 342.4049 deg, Dec -15.2687 to -4.6696 deg
Loaded 5086 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4178 out of 4455 total matches.
Matched with Tycho-2 4455 out of 31665 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.419600
a=0.000000 b=1.000000 c=22.419600
From vast_summary.log: estimated ref. image limiting mag.: -7.65
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.77
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.77
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 31665 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2518 to 342.4049 deg, Dec -15.2687 to -4.6696 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 326.2518 to 342.4049 deg, Dec -15.2687 to -4.6696 deg
Loaded 5086 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4178 out of 4455 total matches.
Matched with Tycho-2 4455 out of 31665 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits -> calib.txt_param_ref_wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits (aperture=4.8)
Read 31663 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2518 to 342.4085 deg, Dec -15.2553 to -4.6543 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 326.2518 to 342.4085 deg, Dec -15.2553 to -4.6543 deg
Loaded 5090 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4191 out of 4451 total matches.
Matched with Tycho-2 4451 out of 31663 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits -> calib.txt_param_ref_wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 35 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
2.2 pix Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits
2.2 pix fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
2.4 pix fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
2.2 pix wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
2.2 pix wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits
Limiting magnitude estimates:
14.8 mag. Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
14.7 mag. Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits
14.6 mag. fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
14.5 mag. fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 14.0 (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.ac2Fs0LXJW (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_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits' -> 'wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
WCS-calibrated image found: wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
Checking if the catalog wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits
WCS catalog name: wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1237, bad_region=4560, passed=31658
Got 31658 stars (including 26107 good ones) from the SExtractor catalog wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat
util/solve_plate_with_UCAC5 got 31658 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 874 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 873 matched stars entering correct_measured_positions(), 869 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 873 matched stars entering correct_measured_positions(), 27571 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 874 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 873 matched stars entering correct_measured_positions(), 27571 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 873 matched stars entering correct_measured_positions(), 27571 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 873 stars left (next iteration limit 960)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits N_match=873 sigma_overall_arcsec=0.388 sigma_q1_arcsec=0.352 sigma_q2_arcsec=0.351 sigma_q3_arcsec=0.432 sigma_q4_arcsec=0.445 n_q1=311 n_q2=145 n_q3=285 n_q4=132 worst_quadrant_to_overall_ratio=1.147
The image catalog is written to wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits -region wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.l4rU3unTJ5 (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_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits' -> 'wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits
WCS-calibrated image found: wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits
Checking if the catalog wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits
WCS catalog name: wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.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=13, blended=1181, bad_region=4531, passed=31650
Got 31650 stars (including 26172 good ones) from the SExtractor catalog wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits.wcscat
util/solve_plate_with_UCAC5 got 31650 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 876 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 875 matched stars entering correct_measured_positions(), 869 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 875 matched stars entering correct_measured_positions(), 27548 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 876 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 875 matched stars entering correct_measured_positions(), 27546 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 875 matched stars entering correct_measured_positions(), 27546 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 875 stars left (next iteration limit 962)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits N_match=875 sigma_overall_arcsec=0.351 sigma_q1_arcsec=0.310 sigma_q2_arcsec=0.354 sigma_q3_arcsec=0.374 sigma_q4_arcsec=0.374 n_q1=308 n_q2=140 n_q3=294 n_q4=133 worst_quadrant_to_overall_ratio=1.066
The image catalog is written to wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits -region wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ApvZJWoExo (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
Checking if the catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
WCS catalog name: wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1617, bad_region=5031, passed=27943
Got 27943 stars (including 21946 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits.wcscat
util/solve_plate_with_UCAC5 got 27943 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
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 880 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 880 matched stars entering correct_measured_positions(), 878 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 880 matched stars entering correct_measured_positions(), 23328 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 880 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 880 matched stars entering correct_measured_positions(), 23328 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 880 matched stars entering correct_measured_positions(), 23329 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 880 stars left (next iteration limit 968)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits N_match=880 sigma_overall_arcsec=0.358 sigma_q1_arcsec=0.337 sigma_q2_arcsec=0.405 sigma_q3_arcsec=0.336 sigma_q4_arcsec=0.313 n_q1=264 n_q2=182 n_q3=253 n_q4=181 worst_quadrant_to_overall_ratio=1.129
The image catalog is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits -region wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.71QpEvyUD3 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
Checking if the catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
WCS catalog name: wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.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=7, blended=1173, bad_region=4632, passed=26642
Got 26642 stars (including 21217 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits.wcscat
util/solve_plate_with_UCAC5 got 26642 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 878 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 878 matched stars entering correct_measured_positions(), 877 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 878 matched stars entering correct_measured_positions(), 22382 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 878 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 878 matched stars entering correct_measured_positions(), 22380 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 878 matched stars entering correct_measured_positions(), 22380 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 878 stars left (next iteration limit 965)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits N_match=878 sigma_overall_arcsec=0.340 sigma_q1_arcsec=0.309 sigma_q2_arcsec=0.388 sigma_q3_arcsec=0.343 sigma_q4_arcsec=0.294 n_q1=265 n_q2=181 n_q3=250 n_q4=182 worst_quadrant_to_overall_ratio=1.140
The image catalog is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits -region wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-46-49_20.00sec_5.00C_LIGHT_0476.fits
Saving fully-calibrated image wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aqr-04-Q2b1x1_061000_TTUQ2b1x1_73954_FHHX8V2T/wcs_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477.fits
Preparing the HTML report for the field Aqr-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:16:43.15 -11:22:28.9: 14.33 +/- 0.13 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:21:07.57 -06:25:53.9: 13.27 +/- 0.06 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits at 22:16:43.15 -11:22:28.9: 14.21 +/- 0.12 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:33:34.58 -14:07:31.0: 14.24 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.26 +/- 0.09
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:24:12.31 -06:31:49.0: 13.71 +/- 0.09 detection
Forced photometry filter REJECTED candidate at 22:16:43.15 -11:22:28.9: ref_mag=14.26 +/- 0.09 new_mean_mag=14.2325 delta=0.03 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:15:58.50 -14:11:38.4: 13.93 +/- 0.11 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:24:06.33 -10:04:22.5: 15.38 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits at 22:21:07.57 -06:25:53.9: 13.27 +/- 0.06 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:13:30.65 -09:07:03.6: 15.50 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.27 +/- 0.04
Forced photometry filter REJECTED candidate at 22:21:07.57 -06:25:53.9: ref_mag=13.27 +/- 0.04 new_mean_mag=13.5540 delta=-0.28 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits at 22:24:12.31 -06:31:49.0: 13.72 +/- 0.09 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:22:24.16 -12:54:15.2: 14.39 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.06
Forced photometry filter REJECTED candidate at 22:24:12.31 -06:31:49.0: ref_mag=13.71 +/- 0.06 new_mean_mag=13.9060 delta=-0.19 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits at 22:15:58.50 -14:11:38.4: 13.94 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.08
Forced photometry filter REJECTED candidate at 22:15:58.50 -14:11:38.4: ref_mag=13.94 +/- 0.08 new_mean_mag=13.8533 delta=0.08 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:27:41.80 -13:32:07.8: 14.73 +/- 0.22 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits at 22:24:06.33 -10:04:22.5: 15.38 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:33:17.83 -13:45:07.6: 14.46 +/- 0.18 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits at 22:33:34.58 -14:07:31.0: 14.19 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.11
Forced photometry filter REJECTED candidate at 22:33:34.58 -14:07:31.0: ref_mag=14.22 +/- 0.11 new_mean_mag=13.8972 delta=0.32 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits at 22:13:30.65 -09:07:03.6: 15.43 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits at 22:22:24.16 -12:54:15.2: 15.01 +/- 0.29 detection
Forced photometry reference-image weighted average: 14.53 +/- 0.14
Forced photometry filter REJECTED candidate at 22:22:24.16 -12:54:15.2: ref_mag=14.53 +/- 0.14 new_mean_mag=14.1984 delta=0.34 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits at 22:27:41.80 -13:32:07.8: 14.97 +/- 0.29 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits at 22:33:17.83 -13:45:07.6: 14.20 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.82 +/- 0.18
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:29:47.64 -14:10:33.0: 14.53 +/- 0.19 detection
Forced photometry filter REJECTED candidate at 22:27:41.80 -13:32:07.8: ref_mag=14.82 +/- 0.18 new_mean_mag=14.1589 delta=0.66 (need > 0.90)
Forced photometry reference-image weighted average: 14.29 +/- 0.11
Forced photometry filter REJECTED candidate at 22:33:17.83 -13:45:07.6: ref_mag=14.29 +/- 0.11 new_mean_mag=14.0011 delta=0.29 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:32:53.16 -13:49:41.2: 14.61 +/- 0.21 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:29:07.96 -13:36:39.9: 14.55 +/- 0.20 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:26:06.06 -07:35:31.4: 14.42 +/- 0.16 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits at 22:29:47.64 -14:10:33.0: 14.64 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.58 +/- 0.14
Forced photometry filter REJECTED candidate at 22:29:47.64 -14:10:33.0: ref_mag=14.58 +/- 0.14 new_mean_mag=14.1764 delta=0.41 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:31:20.40 -14:03:36.2: 14.46 +/- 0.19 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits at 22:32:53.16 -13:49:41.2: 14.53 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.57 +/- 0.14
Forced photometry filter REJECTED candidate at 22:32:53.16 -13:49:41.2: ref_mag=14.57 +/- 0.14 new_mean_mag=14.1562 delta=0.41 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits at 22:29:07.96 -13:36:39.9: 14.52 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.54 +/- 0.14
Forced photometry filter REJECTED candidate at 22:29:07.96 -13:36:39.9: ref_mag=14.54 +/- 0.14 new_mean_mag=14.1892 delta=0.35 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:28:17.26 -13:22:37.9: 14.33 +/- 0.16 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:28:42.00 -13:07:40.0: 14.96 +/- 0.28 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits at 22:31:20.40 -14:03:36.2: 14.39 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.42 +/- 0.13
Forced photometry filter REJECTED candidate at 22:31:20.40 -14:03:36.2: ref_mag=14.42 +/- 0.13 new_mean_mag=14.2437 delta=0.18 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits at 22:26:06.06 -07:35:31.4: 14.77 +/- 0.23 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:35:27.93 -13:43:58.9: 14.69 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.54 +/- 0.13
Forced photometry filter REJECTED candidate at 22:26:06.06 -07:35:31.4: ref_mag=14.54 +/- 0.13 new_mean_mag=14.2365 delta=0.30 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits at 22:28:17.26 -13:22:37.9: 14.48 +/- 0.18 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits at 22:28:42.00 -13:07:40.0: 14.35 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.39 +/- 0.12
Forced photometry filter REJECTED candidate at 22:28:17.26 -13:22:37.9: ref_mag=14.39 +/- 0.12 new_mean_mag=14.1876 delta=0.21 (need > 0.90)
Forced photometry reference-image weighted average: 14.51 +/- 0.14
Forced photometry filter REJECTED candidate at 22:28:42.00 -13:07:40.0: ref_mag=14.51 +/- 0.14 new_mean_mag=14.3503 delta=0.16 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits at 22:35:27.93 -13:43:58.9: 14.33 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.46 +/- 0.14
Forced photometry filter REJECTED candidate at 22:35:27.93 -13:43:58.9: ref_mag=14.46 +/- 0.14 new_mean_mag=14.1729 delta=0.29 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:35:01.12 -11:49:44.8: 14.51 +/- 0.18 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:32:08.87 -10:52:05.1: 14.69 +/- 0.20 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:30:47.12 -10:23:51.5: 14.64 +/- 0.19 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:24:10.87 -13:02:00.6: 14.27 +/- 0.15 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits at 22:35:01.12 -11:49:44.8: 14.58 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.54 +/- 0.13
Forced photometry filter REJECTED candidate at 22:35:01.12 -11:49:44.8: ref_mag=14.54 +/- 0.13 new_mean_mag=14.3851 delta=0.15 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits at 22:32:08.87 -10:52:05.1: 14.52 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.59 +/- 0.13
Forced photometry filter REJECTED candidate at 22:32:08.87 -10:52:05.1: ref_mag=14.59 +/- 0.13 new_mean_mag=14.4481 delta=0.14 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits at 22:24:10.87 -13:02:00.6: 14.16 +/- 0.13 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits at 22:30:47.12 -10:23:51.5: 14.73 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.68 +/- 0.14
Forced photometry reference-image weighted average: 14.21 +/- 0.10
Forced photometry filter REJECTED candidate at 22:30:47.12 -10:23:51.5: ref_mag=14.68 +/- 0.14 new_mean_mag=14.3920 delta=0.29 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:24:10.87 -13:02:00.6: ref_mag=14.21 +/- 0.10 new_mean_mag=14.3133 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410.fits at 22:27:48.81 -07:29:01.9: 12.89 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411.fits at 22:27:48.81 -07:29:01.9: 12.90 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.03
Forced photometry filter KEPT candidate at 22:27:48.81 -07:29:01.9: ref_mag=12.90 +/- 0.03 new_mean_mag=11.9085 delta=0.99 (need > 0.90)
Adding exclusion_list_local.txt__out22312.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55693.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56808.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 52091_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 52091_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 52101_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 52101_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 52102_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 52102_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 52805_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 52805_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 53111_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 53111_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 53168_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 53168_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 53914_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 53914_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 54314_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 54314_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 54696_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 54696_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
**** FOUND 22:20:18.08 -07:49:24.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 55089_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 55089_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 55130_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 55130_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 55132_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 55132_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 55693_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 55693_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 56172_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 56172_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 56334_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 56334_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 56449_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 56449_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 56677_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 56677_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 56808_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 56808_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 56851_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 56851_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 56893_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 56893_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 56897_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 56897_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 56898_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 56898_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 56936_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 56936_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 56966_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 56966_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 57155_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 57155_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 57222_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 57222_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 57229_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 57229_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 57310_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 57310_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 57314_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 57314_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 57321_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 57321_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 57366_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 57366_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 57422_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 57422_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 57500_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 57500_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 23546_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477
The candidate 23546_fd_Aqr-04-Q2b1x1_2026-07-23_05-47-26_20.00sec_5.00C_LIGHT_0477 did not pass the final checks