This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9
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 09 15.2325 2461298.7325 9.37 22:25:10.53 -19:57:12.6
37.07211 -55.84418 galactic Aqr Second-epoch detections are separated by 0.7" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.9 Metis 0 0 0 9.5 -0 -0
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:25:10.53 -19:57:12.6: 14.98 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:25:10.53 -19:57:12.6: 14.81 +/- 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,2461298.7325,9.37,0.05,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 20260915.2325 9.37CV 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 09 15.2325 2461298.7325 11.49 21:55:14.32 -17:39:42.5
36.58202 -48.40528 galactic Cap Second-epoch detections are separated by 0.4" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.100 Hekate 0 -0 0 11.6 0 -0
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 21:55:14.32 -17:39:42.5: 15.06 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 21:55:14.32 -17:39:42.5: 14.81 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.2325* 21 55 14.32 -17 39 42.5 11.5 U Cap 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461298.7325,11.49,0.05,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 20260915.2325 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 15.2325 2461298.7325 13.87 22:26:26.16 -14:55:48.9
45.36919 -54.19106 galactic Aqr Second-epoch detections are separated by 1.6" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.367 Amicitia 0 -1 1 13.9 -0 -0
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:26:26.16 -14:55:48.9: 15.19 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:26:26.16 -14:55:48.9: 15.03 +/- 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,2461298.7325,13.87,0.05,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 20260915.2325 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461212.88358507 21.06.2026 09:12:11.750 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
First image: 2461212.88358507 21.06.2026 09:12:11.750 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
Last image: 2461298.73285020 15.09.2026 05:35:08.257 /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.97
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 4460
Objects passed selection criteria: 4444
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: 3485.75
Average stars matched: 3119.75 (89.5001 %)
Memory usage VmPeak: 230932 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 11 14:55:52 CDT 2026
VaST build number 1.0rc89-210-g97d43bca
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Sep 15 01:09:19 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461212.88358507 21.06.2026 09:12:11.750 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
First image: 2461212.88358507 21.06.2026 09:12:11.750 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
Last image: 2461298.73285020 15.09.2026 05:35:08.257 /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 108
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: 17 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 29332
Objects passed selection criteria: 29257
Measurements per detected object (mean, median, min, max): 3.1 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 3.0 2 4
Average stars detected per image: 23664.2
Average stars matched: 21052.5 (88.9633 %)
Memory usage VmPeak: 250604 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 11 14:55:52 CDT 2026
VaST build number 1.0rc89-210-g97d43bca
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Sep 15 01:10:36 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-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
SExtractor catalog cache: saved Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits.cat to cache
SExtractor catalog cache: saved Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.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-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.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: 2461298.73218764
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-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits exists and is non-empty
wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits exists and is non-empty
wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits exists and is non-empty
wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits (1st reference image)
verification OK: wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
Image size: 937.2'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: 22:13:20.135 -18:00:18.13 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-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits (1st new image)
verification OK: wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits
Image size: 936.9'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:13:20.197 -17:59:56.40 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:13:20.135 -18:00:18.13
Second-epoch image center 22:13:20.197 -17:59:56.40
Angular distance between the image centers 0.0060 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits (2nd new image)
verification OK: wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
Image size: 936.9'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:13:17.402 -17:59:22.09 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:13:20.135 -18:00:18.13
Second-epoch image center 22:13:17.402 -17:59:22.09
Angular distance between the image centers 0.0190 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 22:13:20.197 -17:59:56.40
Second-epoch second image center 22:13:17.402 -17:59:22.09
Angular distance between the image centers 0.01461 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-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits &> /tmp/tmp.oqoMhQVOFV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits &> /tmp/tmp.FXHec7cDJ4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits &> /tmp/tmp.G3hourw7Mp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits &> /tmp/tmp.DRKLIpv0p9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.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-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits and wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.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-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits and wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits.wcscat
Found non-empty wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits and wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits.wcscat
The reference image (wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits) and catalog (wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits.wcscat) found
'wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits.wcscat' -> 'wcsmag.cat'
Read 4587 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 324.9535 to 341.7664 deg, Dec -23.2684 to -12.6150 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 324.9535 to 341.7664 deg, Dec -23.2684 to -12.6150 deg
Loaded 5156 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): 3526 out of 3592 total matches.
Matched with Tycho-2 3592 out of 4587 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.535150
a=0.000000 b=1.000000 c=22.535150
From vast_summary.log: estimated ref. image limiting mag.: -7.97
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.57
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.57
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 4587 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 324.9535 to 341.7664 deg, Dec -23.2684 to -12.6150 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 324.9535 to 341.7664 deg, Dec -23.2684 to -12.6150 deg
Loaded 5156 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): 3526 out of 3592 total matches.
Matched with Tycho-2 3592 out of 4587 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
Forced-photometry filter: calibrated wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits -> calib.txt_param_ref_wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits (aperture=6.2)
Read 3722 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 324.9530 to 341.7678 deg, Dec -23.2603 to -12.6145 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 324.9530 to 341.7678 deg, Dec -23.2603 to -12.6145 deg
Loaded 5151 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): 3021 out of 3064 total matches.
Matched with Tycho-2 3064 out of 3722 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits
Forced-photometry filter: calibrated wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits -> calib.txt_param_ref_wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 7 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
2.2 pix Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits
2.2 pix fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits
2.2 pix fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
Limiting magnitude estimates:
14.6 mag. Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
14.3 mag. Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits
14.8 mag. fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits
14.8 mag. fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 11.3 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.oqoMhQVOFV (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_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.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-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits' -> 'wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
WCS_IMAGE_NAME=wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
WCS-calibrated image found: wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
Checking if the catalog wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits.wcscat corresponding to the image wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits alredy exist and is non-empty...
Catalog wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits.wcscat corresponding to the image wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
WCS catalog name: wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.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=281, bad_region=979, passed=4587
Got 4587 stars (including 3374 good ones) from the SExtractor catalog wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits.wcscat
util/solve_plate_with_UCAC5 got 4587 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 2934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2916 matched stars entering correct_measured_positions(), 2916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2916 matched stars entering correct_measured_positions(), 3784 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 2932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2917 matched stars entering correct_measured_positions(), 3784 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 2917 matched stars entering correct_measured_positions(), 3784 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 2917 stars left (next iteration limit 3207)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits N_match=2917 sigma_overall_arcsec=0.350 sigma_q1_arcsec=0.334 sigma_q2_arcsec=0.386 sigma_q3_arcsec=0.352 sigma_q4_arcsec=0.325 n_q1=984 n_q2=518 n_q3=1005 n_q4=410 worst_quadrant_to_overall_ratio=1.104
The image catalog is written to wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits -region wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.FXHec7cDJ4 (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_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.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-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits' -> 'wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits
WCS_IMAGE_NAME=wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits
WCS-calibrated image found: wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits
Checking if the catalog wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits.wcscat corresponding to the image wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits alredy exist and is non-empty...
Catalog wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits.wcscat corresponding to the image wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits
WCS catalog name: wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.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=233, bad_region=837, passed=3722
Got 3722 stars (including 2702 good ones) from the SExtractor catalog wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits.wcscat
util/solve_plate_with_UCAC5 got 3722 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 2344 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2335 matched stars entering correct_measured_positions(), 2335 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2335 matched stars entering correct_measured_positions(), 3030 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 2344 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2335 matched stars entering correct_measured_positions(), 3030 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 2335 matched stars entering correct_measured_positions(), 3030 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 2335 stars left (next iteration limit 2568)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits N_match=2335 sigma_overall_arcsec=0.424 sigma_q1_arcsec=0.377 sigma_q2_arcsec=0.418 sigma_q3_arcsec=0.478 sigma_q4_arcsec=0.368 n_q1=755 n_q2=396 n_q3=849 n_q4=335 worst_quadrant_to_overall_ratio=1.127
The image catalog is written to wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits -region wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.G3hourw7Mp (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_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.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_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits
WCS-calibrated image found: wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits
Checking if the catalog wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits.wcscat corresponding to the image wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits.wcscat corresponding to the image wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits
WCS catalog name: wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.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=355, bad_region=1355, passed=5108
Got 5108 stars (including 3466 good ones) from the SExtractor catalog wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits.wcscat
util/solve_plate_with_UCAC5 got 5108 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.2 to -12.6)
Done reading UCAC5 zone files...
Matched 3029 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3013 matched stars entering correct_measured_positions(), 3013 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3013 matched stars entering correct_measured_positions(), 3990 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.2 to -12.6)
Done reading UCAC5 zone files...
Matched 3033 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3015 matched stars entering correct_measured_positions(), 3990 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 3015 matched stars entering correct_measured_positions(), 3990 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 3015 stars left (next iteration limit 3314)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3015 robust_rms=7.368 arcsec worst_quadrant_rms=8.431 arcsec
SIP_REFIT: SIP order 3 trial: matched=3015 robust_rms=0.412 arcsec worst_quadrant_rms=0.479 arcsec
SIP_REFIT: SIP order 5 trial: matched=3015 robust_rms=0.346 arcsec worst_quadrant_rms=0.368 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3015 robust_rms_before=0.904 arcsec robust_rms_before_corrected=0.371 arcsec robust_rms_after=0.346 arcsec worst_quadrant_rms_before=0.391 worst_quadrant_rms_after=0.368
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.391 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits N_match=3015 sigma_overall_arcsec=0.395 sigma_q1_arcsec=0.389 sigma_q2_arcsec=0.425 sigma_q3_arcsec=0.389 sigma_q4_arcsec=0.374 n_q1=810 n_q2=689 n_q3=905 n_q4=611 worst_quadrant_to_overall_ratio=1.075
The image catalog is written to wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits -region wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.DRKLIpv0p9 (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_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.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_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
WCS-calibrated image found: wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
Checking if the catalog wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits.wcscat corresponding to the image wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits.wcscat corresponding to the image wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
WCS catalog name: wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.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=341, bad_region=1343, passed=5117
Got 5117 stars (including 3500 good ones) from the SExtractor catalog wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits.wcscat
util/solve_plate_with_UCAC5 got 5117 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.2 to -12.6)
Done reading UCAC5 zone files...
Matched 3058 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3044 matched stars entering correct_measured_positions(), 3044 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3044 matched stars entering correct_measured_positions(), 4013 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.2 to -12.6)
Done reading UCAC5 zone files...
Matched 3060 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3044 matched stars entering correct_measured_positions(), 4013 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 3044 matched stars entering correct_measured_positions(), 4013 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 3044 stars left (next iteration limit 3348)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3044 robust_rms=7.403 arcsec worst_quadrant_rms=8.773 arcsec
SIP_REFIT: SIP order 3 trial: matched=3044 robust_rms=0.384 arcsec worst_quadrant_rms=0.442 arcsec
SIP_REFIT: SIP order 5 trial: matched=3044 robust_rms=0.326 arcsec worst_quadrant_rms=0.337 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3044 robust_rms_before=0.902 arcsec robust_rms_before_corrected=0.334 arcsec robust_rms_after=0.326 arcsec worst_quadrant_rms_before=0.349 worst_quadrant_rms_after=0.337
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.349 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits N_match=3044 sigma_overall_arcsec=0.349 sigma_q1_arcsec=0.340 sigma_q2_arcsec=0.358 sigma_q3_arcsec=0.338 sigma_q4_arcsec=0.343 n_q1=830 n_q2=684 n_q3=923 n_q4=607 worst_quadrant_to_overall_ratio=1.026
The image catalog is written to wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits -region wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits to local_wcs_cache/
'wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits' -> 'local_wcs_cache/wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits'
Saving the final (post-refit) wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits to local_wcs_cache/
'wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits' -> 'local_wcs_cache/wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits'
Saving the final (post-refit) wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits to local_wcs_cache/
'wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits' -> 'local_wcs_cache/wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits'
Saving the final (post-refit) wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits to local_wcs_cache/
'wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits' -> 'local_wcs_cache/wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits sigma_overall=0.350 worst_q_ratio=1.104
ref2=Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits sigma_overall=0.424 worst_q_ratio=1.127
new1=fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits sigma_overall=0.395 worst_q_ratio=1.075
new2=fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits sigma_overall=0.349 worst_q_ratio=1.026
reference average sigma_overall=0.387 worst_q_ratio=1.1155
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404_astrometric_residuals.png (2917 matched stars from wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408_astrometric_residuals.png (2335 matched stars from wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254_astrometric_residuals.png (3015 matched stars from wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255_astrometric_residuals.png (3044 matched stars from wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits'
Saving fully-calibrated image wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits'
Preparing the HTML report for the field Aqr-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:25:10.53 -19:57:12.6: 14.98 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 21:55:14.32 -17:39:42.5: 15.06 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:04:48.43 -15:47:01.3: 11.45 +/- 0.01 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:04:13.69 -18:26:40.2: 11.63 +/- 0.01 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 21:55:14.32 -17:39:42.5: 14.81 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:25:10.53 -19:57:12.6: 14.81 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:04:13.69 -18:26:40.2: 11.66 +/- 0.02 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:04:48.43 -15:47:01.3: 11.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.64 +/- 0.01
Forced photometry reference-image weighted average: 11.45 +/- 0.01
Forced photometry filter REJECTED candidate at 22:04:13.69 -18:26:40.2: ref_mag=11.64 +/- 0.01 new_mean_mag=11.6213 delta=0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:04:48.43 -15:47:01.3: ref_mag=11.45 +/- 0.01 new_mean_mag=11.4111 delta=0.04 (need > 0.90)
Adding exclusion_list_local.txt__out20119.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20666.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20119_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
Preparing report for the candidate 20119_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20126_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 20126_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
**** FOUND 22:19:54.40 -14:24:07.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20367_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 20367_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
**** FOUND 22:18:39.28 -20:54:01.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20519_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 20519_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
**** FOUND 22:24:13.44 -19:47:42.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20615_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 20615_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20666_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
Preparing report for the candidate 20666_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20727_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 20727_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 11s
Prepared the HTML report for the field Aqr-06-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 ####
22:25:10.53 -19:57:12.6
21:55:14.32 -17:39:42.5
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-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
SExtractor catalog cache: saved Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits.cat to cache
SExtractor catalog cache: saved Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.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-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
Creating symlink local_wcs_cache/wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits exists and is non-empty
wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits exists and is non-empty
wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits exists and is non-empty
wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits (1st reference image)
verification OK: wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
Image size: 937.2'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: 22:13:20.135 -18:00:18.13 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-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits (1st new image)
verification OK: wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits
Image size: 936.9'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:13:20.197 -17:59:56.40 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:13:20.135 -18:00:18.13
Second-epoch image center 22:13:20.197 -17:59:56.40
Angular distance between the image centers 0.0060 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits (2nd new image)
verification OK: wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
Image size: 936.9'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:13:17.402 -17:59:22.09 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:13:20.135 -18:00:18.13
Second-epoch image center 22:13:17.402 -17:59:22.09
Angular distance between the image centers 0.0190 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 22:13:20.197 -17:59:56.40
Second-epoch second image center 22:13:17.402 -17:59:22.09
Angular distance between the image centers 0.01461 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-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits &> /tmp/tmp.C78usuWvPN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits &> /tmp/tmp.qQU0oCwt0G
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits &> /tmp/tmp.8BIQsaXVRC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits &> /tmp/tmp.JLe3gfBQ6B
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.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-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits and wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.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-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits and wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits.wcscat
Found non-empty wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits and wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits.wcscat
The reference image (wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits) and catalog (wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits.wcscat) found
'wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits.wcscat' -> 'wcsmag.cat'
Read 27785 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 324.8957 to 341.7911 deg, Dec -23.2683 to -12.6150 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 324.8957 to 341.7911 deg, Dec -23.2683 to -12.6150 deg
Loaded 5172 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): 4205 out of 4428 total matches.
Matched with Tycho-2 4428 out of 27785 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.383400
a=0.000000 b=1.000000 c=22.383400
From vast_summary.log: estimated ref. image limiting mag.: -7.65
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.73
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.73
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 27785 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 324.8957 to 341.7911 deg, Dec -23.2683 to -12.6150 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 324.8957 to 341.7911 deg, Dec -23.2683 to -12.6150 deg
Loaded 5172 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): 4205 out of 4428 total matches.
Matched with Tycho-2 4428 out of 27785 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
Forced-photometry filter: calibrated wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits -> calib.txt_param_ref_wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits (aperture=4.8)
Read 25204 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 324.8815 to 341.8122 deg, Dec -23.2603 to -12.5946 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 324.8815 to 341.8122 deg, Dec -23.2603 to -12.5946 deg
Loaded 5184 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): 4264 out of 4457 total matches.
Matched with Tycho-2 4457 out of 25204 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits
Forced-photometry filter: calibrated wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits -> calib.txt_param_ref_wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 40 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
2.1 pix Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits
2.0 pix fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits
2.1 pix fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
Limiting magnitude estimates:
14.7 mag. Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
14.5 mag. Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits
14.9 mag. fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits
14.9 mag. fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
All-image limiting magnitude estimate: 14.9 (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.C78usuWvPN (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_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.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-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits' -> 'wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
WCS_IMAGE_NAME=wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
WCS-calibrated image found: wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
Checking if the catalog wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits.wcscat corresponding to the image wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits alredy exist and is non-empty...
Catalog wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits.wcscat corresponding to the image wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits
WCS catalog name: wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.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=933, bad_region=3971, passed=27777
Got 27777 stars (including 23053 good ones) from the SExtractor catalog wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits.wcscat
util/solve_plate_with_UCAC5 got 27777 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4357 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4339 matched stars entering correct_measured_positions(), 4339 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4339 matched stars entering correct_measured_positions(), 24779 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4356 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4340 matched stars entering correct_measured_positions(), 24779 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4340 matched stars entering correct_measured_positions(), 24779 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4340 stars left (next iteration limit 4772)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits N_match=4340 sigma_overall_arcsec=0.340 sigma_q1_arcsec=0.324 sigma_q2_arcsec=0.389 sigma_q3_arcsec=0.344 sigma_q4_arcsec=0.328 n_q1=1524 n_q2=702 n_q3=1481 n_q4=633 worst_quadrant_to_overall_ratio=1.146
The image catalog is written to wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits -region wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.qQU0oCwt0G (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_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.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-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits' -> 'wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits
WCS_IMAGE_NAME=wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits
WCS-calibrated image found: wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits
Checking if the catalog wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits.wcscat corresponding to the image wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits alredy exist and is non-empty...
Catalog wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits.wcscat corresponding to the image wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits
WCS catalog name: wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.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=12, blended=739, bad_region=4066, passed=25192
Got 25192 stars (including 20501 good ones) from the SExtractor catalog wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits.wcscat
util/solve_plate_with_UCAC5 got 25192 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4356 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4338 matched stars entering correct_measured_positions(), 4338 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4338 matched stars entering correct_measured_positions(), 22100 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4356 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4338 matched stars entering correct_measured_positions(), 22100 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4338 matched stars entering correct_measured_positions(), 22100 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4338 stars left (next iteration limit 4771)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits N_match=4338 sigma_overall_arcsec=0.419 sigma_q1_arcsec=0.365 sigma_q2_arcsec=0.409 sigma_q3_arcsec=0.491 sigma_q4_arcsec=0.395 n_q1=1506 n_q2=740 n_q3=1451 n_q4=641 worst_quadrant_to_overall_ratio=1.169
The image catalog is written to wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits -region wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.8BIQsaXVRC (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_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.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_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits
WCS-calibrated image found: wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits
Checking if the catalog wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits.wcscat corresponding to the image wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits.wcscat corresponding to the image wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits
WCS catalog name: wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.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=9, blended=1172, bad_region=6077, passed=31243
Got 31243 stars (including 24355 good ones) from the SExtractor catalog wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits.wcscat
util/solve_plate_with_UCAC5 got 31243 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4388 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4370 matched stars entering correct_measured_positions(), 4370 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4370 matched stars entering correct_measured_positions(), 26590 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4390 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4370 matched stars entering correct_measured_positions(), 26590 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4370 matched stars entering correct_measured_positions(), 26590 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4370 stars left (next iteration limit 4807)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4370 robust_rms=7.036 arcsec worst_quadrant_rms=8.493 arcsec
SIP_REFIT: SIP order 3 trial: matched=4370 robust_rms=0.419 arcsec worst_quadrant_rms=0.469 arcsec
SIP_REFIT: SIP order 5 trial: matched=4370 robust_rms=0.351 arcsec worst_quadrant_rms=0.366 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4370 robust_rms_before=0.905 arcsec robust_rms_before_corrected=0.356 arcsec robust_rms_after=0.351 arcsec worst_quadrant_rms_before=0.365 worst_quadrant_rms_after=0.366
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.365 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits N_match=4370 sigma_overall_arcsec=0.378 sigma_q1_arcsec=0.366 sigma_q2_arcsec=0.403 sigma_q3_arcsec=0.376 sigma_q4_arcsec=0.376 n_q1=1219 n_q2=938 n_q3=1368 n_q4=845 worst_quadrant_to_overall_ratio=1.065
The image catalog is written to wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits -region wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.JLe3gfBQ6B (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_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.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_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
WCS-calibrated image found: wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
Checking if the catalog wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits.wcscat corresponding to the image wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits.wcscat corresponding to the image wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
WCS catalog name: wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.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=1146, bad_region=6104, passed=31233
Got 31233 stars (including 24322 good ones) from the SExtractor catalog wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits.wcscat
util/solve_plate_with_UCAC5 got 31233 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4387 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4370 matched stars entering correct_measured_positions(), 4370 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4370 matched stars entering correct_measured_positions(), 26568 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4389 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4370 matched stars entering correct_measured_positions(), 26568 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4370 matched stars entering correct_measured_positions(), 26568 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4370 stars left (next iteration limit 4807)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4370 robust_rms=7.048 arcsec worst_quadrant_rms=8.501 arcsec
SIP_REFIT: SIP order 3 trial: matched=4370 robust_rms=0.397 arcsec worst_quadrant_rms=0.446 arcsec
SIP_REFIT: SIP order 5 trial: matched=4370 robust_rms=0.335 arcsec worst_quadrant_rms=0.344 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4370 robust_rms_before=0.900 arcsec robust_rms_before_corrected=0.333 arcsec robust_rms_after=0.335 arcsec worst_quadrant_rms_before=0.342 worst_quadrant_rms_after=0.344
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.342 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits N_match=4370 sigma_overall_arcsec=0.345 sigma_q1_arcsec=0.330 sigma_q2_arcsec=0.366 sigma_q3_arcsec=0.340 sigma_q4_arcsec=0.343 n_q1=1230 n_q2=938 n_q3=1361 n_q4=841 worst_quadrant_to_overall_ratio=1.059
The image catalog is written to wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits -region wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.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_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-34-11_20.00sec_-0.00C_LIGHT_0254.fits
Saving fully-calibrated image wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.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_2026-09-15_CI_Aqr-06-Q2b1x1_010639_TTUQ2b1x1_1118186_pUp2v5I9/wcs_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255.fits
Preparing the HTML report for the field Aqr-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:30:29.19 -21:18:04.6: 14.21 +/- 0.17 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:22:36.18 -21:44:09.5: 13.87 +/- 0.12 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:26:43.91 -15:17:43.4: 13.93 +/- 0.11 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:26:26.16 -14:55:48.9: 15.19 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 21:56:18.59 -17:08:40.6: 13.86 +/- 0.10 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:17:02.51 -21:13:39.4: 13.02 +/- 0.05 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:04:55.85 -21:53:20.3: 14.16 +/- 0.15 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:18:10.53 -22:03:44.0: 14.46 +/- 0.20 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:31:54.48 -21:00:11.9: 14.19 +/- 0.17 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:23:49.37 -22:10:02.8: 14.07 +/- 0.16 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:30:29.19 -21:18:04.6: 14.26 +/- 0.21 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:17:02.51 -21:13:39.4: 13.19 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.13
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:22:36.18 -21:44:09.5: 13.66 +/- 0.11 detection
Forced photometry filter REJECTED candidate at 22:30:29.19 -21:18:04.6: ref_mag=14.23 +/- 0.13 new_mean_mag=14.0448 delta=0.18 (need > 0.90)
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:26:43.91 -15:17:43.4: 13.85 +/- 0.12 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 21:56:18.59 -17:08:40.6: 13.63 +/- 0.10 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:26:26.16 -14:55:48.9: 15.03 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.75 +/- 0.07
Forced photometry reference-image weighted average: 13.07 +/- 0.04
Forced photometry reference-image weighted average: 13.76 +/- 0.08
Forced photometry reference-image weighted average: 13.90 +/- 0.08
Forced photometry filter REJECTED candidate at 21:56:18.59 -17:08:40.6: ref_mag=13.75 +/- 0.07 new_mean_mag=13.8798 delta=-0.13 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:17:02.51 -21:13:39.4: ref_mag=13.07 +/- 0.04 new_mean_mag=13.3705 delta=-0.30 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:22:36.18 -21:44:09.5: ref_mag=13.76 +/- 0.08 new_mean_mag=13.8589 delta=-0.10 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:26:43.91 -15:17:43.4: ref_mag=13.90 +/- 0.08 new_mean_mag=14.0592 delta=-0.16 (need > 0.90)
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:04:55.85 -21:53:20.3: 14.55 +/- 0.26 detection
Forced photometry reference-image weighted average: 14.26 +/- 0.13
Forced photometry filter REJECTED candidate at 22:04:55.85 -21:53:20.3: ref_mag=14.26 +/- 0.13 new_mean_mag=14.0568 delta=0.20 (need > 0.90)
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:18:10.53 -22:03:44.0: 14.23 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.14
Forced photometry filter REJECTED candidate at 22:18:10.53 -22:03:44.0: ref_mag=14.35 +/- 0.14 new_mean_mag=14.0876 delta=0.26 (need > 0.90)
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:23:49.37 -22:10:02.8: 14.18 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.11 +/- 0.12
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:31:54.48 -21:00:11.9: 14.32 +/- 0.23 detection
Forced photometry filter REJECTED candidate at 22:23:49.37 -22:10:02.8: ref_mag=14.11 +/- 0.12 new_mean_mag=13.9482 delta=0.17 (need > 0.90)
Forced photometry reference-image weighted average: 14.23 +/- 0.14
Forced photometry filter REJECTED candidate at 22:31:54.48 -21:00:11.9: ref_mag=14.23 +/- 0.14 new_mean_mag=14.0082 delta=0.22 (need > 0.90)
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:29:08.18 -21:46:21.9: 14.64 +/- 0.25 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:26:54.37 -22:04:22.8: 14.76 +/- 0.30 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:22:29.76 -21:55:54.2: 14.18 +/- 0.15 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:25:00.13 -21:53:58.7: 14.04 +/- 0.14 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:20:00.94 -21:59:49.9: 14.10 +/- 0.16 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:25:45.69 -16:56:29.4: 14.46 +/- 0.18 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:20:56.08 -14:54:52.4: 13.91 +/- 0.12 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:11:46.40 -22:03:34.0: 14.22 +/- 0.16 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:32:20.65 -19:46:10.9: 14.31 +/- 0.17 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:20:00.94 -21:59:49.9: 13.86 +/- 0.16 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:25:00.13 -21:53:58.7: 14.48 +/- 0.26 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.11
Forced photometry filter REJECTED candidate at 22:20:00.94 -21:59:49.9: ref_mag=13.98 +/- 0.11 new_mean_mag=14.0354 delta=-0.06 (need > 0.90)
Forced photometry reference-image weighted average: 14.14 +/- 0.12
Forced photometry filter REJECTED candidate at 22:25:00.13 -21:53:58.7: ref_mag=14.14 +/- 0.12 new_mean_mag=14.1333 delta=0.00 (need > 0.90)
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:26:54.37 -22:04:22.8: 14.34 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.50 +/- 0.18
Forced photometry filter REJECTED candidate at 22:26:54.37 -22:04:22.8: ref_mag=14.50 +/- 0.18 new_mean_mag=14.1307 delta=0.37 (need > 0.90)
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:29:08.18 -21:46:21.9: 14.04 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.14
Forced photometry filter REJECTED candidate at 22:29:08.18 -21:46:21.9: ref_mag=14.23 +/- 0.14 new_mean_mag=14.1604 delta=0.07 (need > 0.90)
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:22:29.76 -21:55:54.2: 14.37 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.24 +/- 0.13
Forced photometry filter REJECTED candidate at 22:22:29.76 -21:55:54.2: ref_mag=14.24 +/- 0.13 new_mean_mag=14.0022 delta=0.24 (need > 0.90)
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:25:45.69 -16:56:29.4: 14.17 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.31 +/- 0.13
Forced photometry filter REJECTED candidate at 22:25:45.69 -16:56:29.4: ref_mag=14.31 +/- 0.13 new_mean_mag=14.1559 delta=0.15 (need > 0.90)
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:20:56.08 -14:54:52.4: 14.05 +/- 0.17 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.10
Forced photometry filter REJECTED candidate at 22:20:56.08 -14:54:52.4: ref_mag=13.95 +/- 0.10 new_mean_mag=14.0351 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:11:46.40 -22:03:34.0: 14.18 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.20 +/- 0.12
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:32:20.65 -19:46:10.9: 14.28 +/- 0.21 detection
Forced photometry filter REJECTED candidate at 22:11:46.40 -22:03:34.0: ref_mag=14.20 +/- 0.12 new_mean_mag=14.0341 delta=0.17 (need > 0.90)
Forced photometry reference-image weighted average: 14.30 +/- 0.14
Forced photometry filter REJECTED candidate at 22:32:20.65 -19:46:10.9: ref_mag=14.30 +/- 0.14 new_mean_mag=14.2316 delta=0.07 (need > 0.90)
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:26:02.30 -21:28:53.8: 14.17 +/- 0.16 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:32:10.97 -20:57:42.5: 14.29 +/- 0.18 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:10:38.44 -22:15:43.2: 14.45 +/- 0.21 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:30:20.57 -22:02:17.7: 14.22 +/- 0.18 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:23:56.19 -13:58:41.2: 14.25 +/- 0.14 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:21:18.14 -18:34:44.5: 14.32 +/- 0.15 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:26:30.95 -22:09:42.5: 14.18 +/- 0.17 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:28:12.25 -14:35:26.9: 14.13 +/- 0.13 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:10:38.44 -22:15:43.2: 14.62 +/- 0.28 detection
Forced photometry reference-image weighted average: 14.51 +/- 0.17
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:26:02.30 -21:28:53.8: 14.41 +/- 0.24 detection
Forced photometry filter REJECTED candidate at 22:10:38.44 -22:15:43.2: ref_mag=14.51 +/- 0.17 new_mean_mag=14.1774 delta=0.33 (need > 0.90)
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:30:20.57 -22:02:17.7: 14.09 +/- 0.19 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:20:32.91 -21:49:45.1: 14.48 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.24 +/- 0.13
Forced photometry filter REJECTED candidate at 22:26:02.30 -21:28:53.8: ref_mag=14.24 +/- 0.13 new_mean_mag=14.1324 delta=0.11 (need > 0.90)
Forced photometry reference-image weighted average: 14.16 +/- 0.13
Forced photometry filter REJECTED candidate at 22:30:20.57 -22:02:17.7: ref_mag=14.16 +/- 0.13 new_mean_mag=14.1097 delta=0.05 (need > 0.90)
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:23:56.19 -13:58:41.2: 14.14 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.20 +/- 0.11
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:32:10.97 -20:57:42.5: 14.35 +/- 0.24 detection
Forced photometry filter REJECTED candidate at 22:23:56.19 -13:58:41.2: ref_mag=14.20 +/- 0.11 new_mean_mag=14.0924 delta=0.11 (need > 0.90)
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:21:18.14 -18:34:44.5: 14.19 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.26 +/- 0.11
Forced photometry reference-image weighted average: 14.31 +/- 0.15
Forced photometry filter REJECTED candidate at 22:21:18.14 -18:34:44.5: ref_mag=14.26 +/- 0.11 new_mean_mag=14.2066 delta=0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:32:10.97 -20:57:42.5: ref_mag=14.31 +/- 0.15 new_mean_mag=14.0989 delta=0.22 (need > 0.90)
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:26:30.95 -22:09:42.5: 14.60 +/- 0.30 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.15
Forced photometry filter REJECTED candidate at 22:26:30.95 -22:09:42.5: ref_mag=14.28 +/- 0.15 new_mean_mag=14.0198 delta=0.26 (need > 0.90)
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:28:12.25 -14:35:26.9: 14.13 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.10
Forced photometry filter REJECTED candidate at 22:28:12.25 -14:35:26.9: ref_mag=14.13 +/- 0.10 new_mean_mag=14.0668 delta=0.06 (need > 0.90)
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:20:32.91 -21:49:45.1: 14.57 +/- 0.28 detection
Forced photometry reference-image weighted average: 14.51 +/- 0.17
Forced photometry filter REJECTED candidate at 22:20:32.91 -21:49:45.1: ref_mag=14.51 +/- 0.17 new_mean_mag=14.2348 delta=0.28 (need > 0.90)
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:17:09.60 -21:37:49.9: 14.23 +/- 0.16 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:23:35.62 -21:30:44.5: 14.25 +/- 0.16 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:07:49.94 -16:58:10.5: 14.08 +/- 0.12 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:05:38.50 -21:54:54.5: 13.97 +/- 0.13 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 21:56:38.78 -13:43:54.3: 14.25 +/- 0.14 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:17:09.60 -21:37:49.9: 14.53 +/- 0.25 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:23:35.62 -21:30:44.5: 14.61 +/- 0.29 detection
Forced photometry reference-image weighted average: 14.32 +/- 0.13
Forced photometry filter REJECTED candidate at 22:17:09.60 -21:37:49.9: ref_mag=14.32 +/- 0.13 new_mean_mag=14.2424 delta=0.07 (need > 0.90)
Forced photometry reference-image weighted average: 14.34 +/- 0.14
Forced photometry filter REJECTED candidate at 22:23:35.62 -21:30:44.5: ref_mag=14.34 +/- 0.14 new_mean_mag=14.2290 delta=0.11 (need > 0.90)
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-21_04-12-11_20.00sec_4.90C_LIGHT_0404.fits at 22:09:42.24 -14:34:55.7: 14.12 +/- 0.14 detection
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:07:49.94 -16:58:10.5: 13.98 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.09
Forced photometry filter REJECTED candidate at 22:07:49.94 -16:58:10.5: ref_mag=14.04 +/- 0.09 new_mean_mag=14.1511 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:05:38.50 -21:54:54.5: 14.24 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.05 +/- 0.11
Forced photometry filter REJECTED candidate at 22:05:38.50 -21:54:54.5: ref_mag=14.05 +/- 0.11 new_mean_mag=14.0842 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 21:56:38.78 -13:43:54.3: 14.24 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.11
Forced photometry filter REJECTED candidate at 21:56:38.78 -13:43:54.3: ref_mag=14.25 +/- 0.11 new_mean_mag=14.2011 delta=0.04 (need > 0.90)
Forced photometry on wcs_Aqr-06-Q2b1x1_2026-06-23_04-33-50_20.00sec_5.00C_LIGHT_0408.fits at 22:09:42.24 -14:34:55.7: 14.15 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.10
Forced photometry filter REJECTED candidate at 22:09:42.24 -14:34:55.7: ref_mag=14.13 +/- 0.10 new_mean_mag=14.1405 delta=-0.01 (need > 0.90)
Adding exclusion_list_local.txt__out34625.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30883_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 30883_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30889_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 30889_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30992_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 30992_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
**** FOUND 22:25:10.54 -19:57:12.6 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31416_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 31416_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
**** FOUND 22:24:13.44 -19:47:42.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31553_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 31553_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
**** FOUND 21:55:14.33 -17:39:42.5 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34484_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 34484_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34625_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
Preparing report for the candidate 34625_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34859_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 34859_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34879_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 34879_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34893_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 34893_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34987_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 34987_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34997_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 34997_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35014_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 35014_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35016_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 35016_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35019_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 35019_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35066_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 35066_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35107_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 35107_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35123_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 35123_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35146_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 35146_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35153_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 35153_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35161_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 35161_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35164_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 35164_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35175_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 35175_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35186_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 35186_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35232_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 35232_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35234_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 35234_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35240_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 35240_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35242_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 35242_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35257_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 35257_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35262_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 35262_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35264_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 35264_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35278_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 35278_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35280_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 35280_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35284_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 35284_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35299_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 35299_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35370_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 35370_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35406_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 35406_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23288_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 23288_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
**** FOUND 22:19:54.41 -14:24:07.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04953_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 04953_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks
**** FOUND 22:18:39.28 -20:54:02.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04448_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255
The candidate 04448_fd_Aqr-06-Q2b1x1_2026-09-15_00-35-08_20.00sec_-0.00C_LIGHT_0255 did not pass the final checks