This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx
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 05 26.2248 2461186.7248 11.86 19:06:34.52 +00:25:39.4
35.04049 -3.17212 galactic Aql Second-epoch detections are separated by 1.7" and 6.5 pix
The object was found in VSX 1" NSVS 13980599
Type: SR
# Max. Min./Amp. JD0 Period
14.222 g Y 0.316 g 2458650.64710 107.245747900000
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 19:06:34.52 +00:25:39.4: 12.80 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 19:06:34.52 +00:25:39.4: 12.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 13980599,2461186.7248,11.86,0.05,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
NSVS 13980599 20260526.2248 11.86CV 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 05 26.2248 2461186.7248 11.49 18:42:31.59 -03:35:39.1
28.71774 0.34055 galactic Aql Second-epoch detections are separated by 0.4" and 6.2 pix
The object was found in VSX 2" ASAS J184232-0335.6
Type: MISC
# Max. Min./Amp. JD0 Period
13.080 V Y 0.570 V 2452316.00000 97.999413000000 M8
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:42:31.59 -03:35:39.1: 12.39 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:42:31.59 -03:35:39.1: 12.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.02
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
ASAS J184232-0335.6,2461186.7248,11.49,0.05,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
ASAS J184232-0335.6 20260526.2248 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461146.82488052 16.04.2026 07:47:39.677 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
First image: 2461146.82488052 16.04.2026 07:47:39.677 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
Last image: 2461186.72507451 26.05.2026 05:23:56.438 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.13
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: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6483
Objects passed selection criteria: 6475
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 4094.25
Average stars matched: 3948.25 (96.434 %)
Memory usage VmPeak: 113860 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue May 26 00:28:26 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: 2461146.82488052 16.04.2026 07:47:39.677 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
First image: 2461146.82488052 16.04.2026 07:47:39.677 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
Last image: 2461186.72507451 26.05.2026 05:23:56.438 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 10
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.79
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: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 71651
Objects passed selection criteria: 71462
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 48076
Average stars matched: 45668.8 (94.9928 %)
Memory usage VmPeak: 186932 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue May 26 00:31:27 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 --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
SExtractor catalog cache: saved Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat to cache
SExtractor catalog cache: saved Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.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: 2461186.72459373
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits exists and is non-empty
Saving wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits to local_wcs_cache/
'wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits' -> 'local_wcs_cache/wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits'
wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits exists and is non-empty
Saving wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits to local_wcs_cache/
'wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits' -> 'local_wcs_cache/wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits'
wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits exists and is non-empty
Saving wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits to local_wcs_cache/
'wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits' -> 'local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits'
wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits exists and is non-empty
Saving wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits to local_wcs_cache/
'wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits' -> 'local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits (1st reference image)
verification OK: wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
Image size: 943.0'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:51:21.238 -02:00:51.43 J2000 4789.000 3195.000
###################################
The image scale is 5.91"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits (1st new image)
verification OK: wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits
Image size: 938.3'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 18:51:38.815 -02:01:00.81 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:51:21.238 -02:00:51.43
Second-epoch image center 18:51:38.815 -02:01:00.81
Angular distance between the image centers 0.0732 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits (2nd new image)
verification OK: wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
Image size: 938.2'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 18:51:38.179 -02:01:36.89 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:51:21.238 -02:00:51.43
Second-epoch image center 18:51:38.179 -02:01:36.89
Angular distance between the image centers 0.0717 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 18:51:38.815 -02:01:00.81
Second-epoch second image center 18:51:38.179 -02:01:36.89
Angular distance between the image centers 0.01037 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits &> /tmp/tmp.T5Dr2BCTqF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits &> /tmp/tmp.WrA8rQ5XKH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits &> /tmp/tmp.Lwhi92nmIg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits &> /tmp/tmp.W20eRQLuMt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits and wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits and wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat
Found non-empty wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits and wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat
The reference image (wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits) and catalog (wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat) found
'wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat' -> 'wcsmag.cat'
Read 10727 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.6382 to 291.0089 deg, Dec -7.7289 to +3.7311 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 274.6382 to 291.0089 deg, Dec -7.7289 to 3.7311 deg
Loaded 10967 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): 6449 out of 6736 total matches.
Matched with Tycho-2 6736 out of 10727 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.627900
a=0.000000 b=1.000000 c=22.627900
From vast_summary.log: estimated ref. image limiting mag.: -8.13
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.50
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.50
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 10727 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.6382 to 291.0089 deg, Dec -7.7289 to +3.7311 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 274.6382 to 291.0089 deg, Dec -7.7289 to 3.7311 deg
Loaded 10967 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): 6449 out of 6736 total matches.
Matched with Tycho-2 6736 out of 10727 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits:
Forced-photometry filter: calibrated wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits -> calib.txt_param_ref_wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits (aperture=6.2)
Read 10007 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.9538 to 290.8167 deg, Dec -7.2966 to +3.3664 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 274.9538 to 290.8167 deg, Dec -7.2966 to 3.3664 deg
Loaded 9632 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): 6263 out of 6516 total matches.
Matched with Tycho-2 6516 out of 10007 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits:
Forced-photometry filter: calibrated wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits -> calib.txt_param_ref_wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits (aperture=6.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
2.4 pix Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
2.3 pix fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits
2.3 pix fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
2.2 pix wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
2.4 pix wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
Limiting magnitude estimates:
14.5 mag. Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
14.3 mag. Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
11.4 mag. fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits
11.4 mag. fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
All-image limiting magnitude estimate: 11.4 (SNR ) 9.4 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.T5Dr2BCTqF (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits' -> 'wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
WCS-calibrated image found: wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
Checking if the catalog wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
WCS catalog name: wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=845, passed=10727
Got 10727 stars (including 9870 good ones) from the SExtractor catalog wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat
util/solve_plate_with_UCAC5 got 10727 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.0'
Seting catalog search parameters based on the expected field of view 943.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013097 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010478 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 10553 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 10550 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 10550 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits N_match=943 sigma_overall_arcsec=0.369 sigma_q1_arcsec=0.357 sigma_q2_arcsec=0.444 sigma_q3_arcsec=0.365 sigma_q4_arcsec=0.339 n_q1=197 n_q2=242 n_q3=217 n_q4=287 worst_quadrant_to_overall_ratio=1.202
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits -region wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.WrA8rQ5XKH (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_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits' -> 'wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
WCS-calibrated image found: wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
Checking if the catalog wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
WCS catalog name: wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=756, passed=10007
Got 10007 stars (including 9239 good ones) from the SExtractor catalog wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat
util/solve_plate_with_UCAC5 got 10007 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (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 0.010423 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 9836 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 9834 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 9834 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits N_match=951 sigma_overall_arcsec=0.602 sigma_q1_arcsec=0.535 sigma_q2_arcsec=0.709 sigma_q3_arcsec=0.574 sigma_q4_arcsec=0.602 n_q1=197 n_q2=247 n_q3=210 n_q4=297 worst_quadrant_to_overall_ratio=1.177
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits -region wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Lwhi92nmIg (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_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.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_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=75, passed=916
Got 916 stars (including 840 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits.cat
util/solve_plate_with_UCAC5 got 916 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (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 0.010426 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 794 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 791 matched stars entering correct_measured_positions(), 757 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 791 matched stars entering correct_measured_positions(), 872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 795 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 792 matched stars entering correct_measured_positions(), 868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 792 matched stars entering correct_measured_positions(), 868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 792 stars left (next iteration limit 870)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits N_match=792 sigma_overall_arcsec=0.678 sigma_q1_arcsec=0.624 sigma_q2_arcsec=0.945 sigma_q3_arcsec=0.574 sigma_q4_arcsec=0.801 n_q1=210 n_q2=97 n_q3=208 n_q4=277 worst_quadrant_to_overall_ratio=1.393
The image catalog is written to wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits -region wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.W20eRQLuMt (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_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.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_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=77, passed=906
Got 906 stars (including 829 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits.cat
util/solve_plate_with_UCAC5 got 906 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 785 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 782 matched stars entering correct_measured_positions(), 743 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 782 matched stars entering correct_measured_positions(), 857 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 786 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 783 matched stars entering correct_measured_positions(), 858 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 783 matched stars entering correct_measured_positions(), 858 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 783 stars left (next iteration limit 860)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits N_match=783 sigma_overall_arcsec=0.684 sigma_q1_arcsec=0.644 sigma_q2_arcsec=0.822 sigma_q3_arcsec=0.554 sigma_q4_arcsec=0.810 n_q1=205 n_q2=94 n_q3=201 n_q4=283 worst_quadrant_to_overall_ratio=1.200
The image catalog is written to wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits -region wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits sigma_overall=0.369 worst_q_ratio=1.202
ref2=Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits sigma_overall=0.602 worst_q_ratio=1.177
new1=fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits sigma_overall=0.678 worst_q_ratio=1.393
new2=fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits sigma_overall=0.684 worst_q_ratio=1.200
reference average sigma_overall=0.4855 worst_q_ratio=1.1895
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245_astrometric_residuals.png (943 matched stars from wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119_astrometric_residuals.png (951 matched stars from wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154_astrometric_residuals.png (792 matched stars from wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155_astrometric_residuals.png (783 matched stars from wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits'
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits'
Preparing the HTML report for the field Aql-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Aql-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
SExtractor catalog cache: saved Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat to cache
SExtractor catalog cache: saved Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
Creating symlink local_wcs_cache/wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits exists and is non-empty
wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits exists and is non-empty
wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits exists and is non-empty
wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits (1st reference image)
verification OK: wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
Image size: 943.0'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:51:21.238 -02:00:51.43 J2000 4789.000 3195.000
###################################
The image scale is 5.91"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits (1st new image)
verification OK: wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits
Image size: 938.3'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 18:51:38.815 -02:01:00.81 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:51:21.238 -02:00:51.43
Second-epoch image center 18:51:38.815 -02:01:00.81
Angular distance between the image centers 0.0732 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits (2nd new image)
verification OK: wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
Image size: 938.2'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 18:51:38.179 -02:01:36.89 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:51:21.238 -02:00:51.43
Second-epoch image center 18:51:38.179 -02:01:36.89
Angular distance between the image centers 0.0717 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 18:51:38.815 -02:01:00.81
Second-epoch second image center 18:51:38.179 -02:01:36.89
Angular distance between the image centers 0.01037 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits &> /tmp/tmp.oj7qrrI9YK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits &> /tmp/tmp.dXQDbnKOcE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits &> /tmp/tmp.L3xHRf7LKm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits &> /tmp/tmp.4CYRP6FFM6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits and wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits and wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat
Found non-empty wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits and wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat
The reference image (wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits) and catalog (wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat) found
'wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat' -> 'wcsmag.cat'
Read 122602 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.5985 to 291.0381 deg, Dec -7.7684 to +3.7641 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 274.5985 to 291.0381 deg, Dec -7.7684 to 3.7641 deg
Loaded 11083 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): 6807 out of 8428 total matches.
Matched with Tycho-2 8428 out of 122602 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.414100
a=0.000000 b=1.000000 c=22.414100
From vast_summary.log: estimated ref. image limiting mag.: -7.79
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.62
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.62
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 122602 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.5985 to 291.0381 deg, Dec -7.7684 to +3.7641 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 274.5985 to 291.0381 deg, Dec -7.7684 to 3.7641 deg
Loaded 11083 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): 6807 out of 8428 total matches.
Matched with Tycho-2 8428 out of 122602 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits:
Forced-photometry filter: calibrated wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits -> calib.txt_param_ref_wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits (aperture=4.4)
Read 111944 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.9350 to 290.8262 deg, Dec -7.3187 to +3.3664 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 274.9350 to 290.8262 deg, Dec -7.3187 to 3.3664 deg
Loaded 9679 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): 6784 out of 8259 total matches.
Matched with Tycho-2 8259 out of 111944 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits:
Forced-photometry filter: calibrated wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits -> calib.txt_param_ref_wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
2.2 pix Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
2.1 pix fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits
2.1 pix fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
2.1 pix wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
2.2 pix wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
Limiting magnitude estimates:
14.6 mag. Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
14.5 mag. Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
12.3 mag. fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits
12.2 mag. fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
All-image limiting magnitude estimate: 12.2 (SNR ) 11.9 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.oj7qrrI9YK (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits' -> 'wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
WCS-calibrated image found: wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
Checking if the catalog wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
WCS catalog name: wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=12771, passed=122591
Got 122591 stars (including 109593 good ones) from the SExtractor catalog wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat
util/solve_plate_with_UCAC5 got 122591 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.0'
Seting catalog search parameters based on the expected field of view 943.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013097 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010478 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.8 to 3.8)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 121311 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.8 to 3.8)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 121312 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 121310 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits N_match=945 sigma_overall_arcsec=0.380 sigma_q1_arcsec=0.357 sigma_q2_arcsec=0.424 sigma_q3_arcsec=0.353 sigma_q4_arcsec=0.388 n_q1=205 n_q2=239 n_q3=224 n_q4=277 worst_quadrant_to_overall_ratio=1.116
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits -region wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.dXQDbnKOcE (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_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits' -> 'wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
WCS-calibrated image found: wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
Checking if the catalog wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
WCS catalog name: wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=11221, passed=111923
Got 111923 stars (including 100547 good ones) from the SExtractor catalog wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat
util/solve_plate_with_UCAC5 got 111923 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (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 0.010423 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 110179 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 110179 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 110179 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits N_match=951 sigma_overall_arcsec=0.602 sigma_q1_arcsec=0.503 sigma_q2_arcsec=0.654 sigma_q3_arcsec=0.591 sigma_q4_arcsec=0.639 n_q1=187 n_q2=262 n_q3=205 n_q4=297 worst_quadrant_to_overall_ratio=1.086
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits -region wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.L3xHRf7LKm (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_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.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_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=235, passed=11590
Got 11590 stars (including 11339 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits.cat
util/solve_plate_with_UCAC5 got 11590 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (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 0.010426 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 11088 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 11082 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 11082 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits N_match=935 sigma_overall_arcsec=0.650 sigma_q1_arcsec=0.586 sigma_q2_arcsec=0.850 sigma_q3_arcsec=0.572 sigma_q4_arcsec=0.740 n_q1=254 n_q2=96 n_q3=258 n_q4=327 worst_quadrant_to_overall_ratio=1.309
The image catalog is written to wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits -region wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.4CYRP6FFM6 (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_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.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_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=241, passed=11719
Got 11719 stars (including 11454 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits.cat
util/solve_plate_with_UCAC5 got 11719 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 11188 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 11186 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 11186 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 937 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits N_match=937 sigma_overall_arcsec=0.655 sigma_q1_arcsec=0.642 sigma_q2_arcsec=0.712 sigma_q3_arcsec=0.567 sigma_q4_arcsec=0.773 n_q1=256 n_q2=92 n_q3=258 n_q4=331 worst_quadrant_to_overall_ratio=1.180
The image catalog is written to wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits -region wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.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_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-14_20.00sec_4.90C_LIGHT_0154.fits
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.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_2026-05-26_CI_Aql-03-Q2b1x1_002452_TTUQ2b1x1_2676402_BSG0l4Dx/wcs_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155.fits
Preparing the HTML report for the field Aql-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:43:26.36 -05:46:21.8: 11.71 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:42:31.59 -03:35:39.1: 12.39 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 19:06:34.52 +00:25:39.4: 12.80 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:43:26.36 -05:46:21.8: 11.67 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.69 +/- 0.02
Forced photometry filter REJECTED candidate at 18:43:26.36 -05:46:21.8: ref_mag=11.69 +/- 0.02 new_mean_mag=11.2381 delta=0.45 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:42:31.59 -03:35:39.1: 12.66 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 19:06:34.52 +00:25:39.4: 12.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.02
Forced photometry reference-image weighted average: 12.77 +/- 0.03
Forced photometry filter KEPT candidate at 18:42:31.59 -03:35:39.1: ref_mag=12.48 +/- 0.02 new_mean_mag=11.4941 delta=0.99 (need > 0.90)
Forced photometry filter KEPT candidate at 19:06:34.52 +00:25:39.4: ref_mag=12.77 +/- 0.03 new_mean_mag=11.8181 delta=0.95 (need > 0.90)
Adding exclusion_list_local.txt__out53617.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99311.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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
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Considering the candidate 142184_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155
The candidate 142184_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155 did not pass the final checks
**** FOUND 18:47:01.83 -04:44:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142189_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155
The candidate 142189_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155 did not pass the final checks
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Considering the candidate 142191_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155
The candidate 142191_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155 did not pass the final checks
**** FOUND 19:03:37.47 +01:48:45.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 99311_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155
Preparing report for the candidate 99311_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155
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Considering the candidate 53617_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155
Preparing report for the candidate 53617_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155
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Considering the candidate 39367_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155
The candidate 39367_fd_Aql-03-Q2b1x1_2026-05-26_00-23-56_20.00sec_4.90C_LIGHT_0155 did not pass the final checks