This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj
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 03 30.3877 2461129.8877 10.07 18:51:04.31 -06:16:13.5
27.30535 -2.77362 galactic Sct Second-epoch detections are separated by 6.0" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | GDS_J1851019-061616 | 18:51:03.41 -06:16:20.2 (Gaia DR3) | VAR (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: K2III 1922ApJ....55...85L NGC 6705 Str 423
Check this position in TNS.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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1851019-061616,2461129.8877,10.07,0.05,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
GDS_J1851019-061616 20260330.3877 10.07CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:51:04.31 -06:16:13.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20_00sec_-10_00C_LIGHT_0334_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20_00sec_-10_00C_LIGHT_0333_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20_00sec_-10_00C_LIGHT_0334_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20_00sec_-10_00C_LIGHT_0333_fits__*pix.png animation_v2.gif
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4265267670238271360,2461129.8877,12.50,0.05,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
Gaia DR3 4265267670238271360 20260330.3877 12.50CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:51:58.16 -01:17:58.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20_00sec_-10_00C_LIGHT_0334_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20_00sec_-10_00C_LIGHT_0333_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20_00sec_-10_00C_LIGHT_0334_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20_00sec_-10_00C_LIGHT_0333_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461099.00015142 27.02.2026 12:00:03.083 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
First image: 2461099.00015142 27.02.2026 12:00:03.083 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Last image: 2461129.88801414 30.03.2026 09:18:34.422 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.06
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): 9778
Objects passed selection criteria: 9739
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 7152.25
Average stars matched: 6932.75 (96.931 %)
Memory usage VmPeak: 116672 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Mar 30 04:20:56 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: 2461099.00015142 27.02.2026 12:00:03.083 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
First image: 2461099.00015142 27.02.2026 12:00:03.083 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Last image: 2461129.88801414 30.03.2026 09:18:34.422 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 45
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.77
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: 29 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): 115190
Objects passed selection criteria: 114920
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 87208
Average stars matched: 83381.8 (95.6125 %)
Memory usage VmPeak: 1956020 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Mar 30 04:23:35 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_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
SExtractor catalog cache: saved Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat to cache
SExtractor catalog cache: saved Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.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: 2461129.88738063
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'
Plate-solving the images
wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits exists and is non-empty
Saving wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits to local_wcs_cache/
'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits' -> 'local_wcs_cache/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits'
wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits exists and is non-empty
Saving wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits to local_wcs_cache/
'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits' -> 'local_wcs_cache/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits'
wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits exists and is non-empty
Saving wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits to local_wcs_cache/
'wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits' -> 'local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits'
wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits exists and is non-empty
Saving wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits to local_wcs_cache/
'wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits' -> 'local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:51:25.226 -01:59:55.32
Second-epoch image center 18:51:26.598 -02:02:30.53
Angular distance between the image centers 0.04 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:51:25.226 -01:59:55.32
Second-epoch image center 18:51:23.549 -02:03:12.56
Angular distance between the image centers 0.06 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 18:51:26.598 -02:02:30.53
Second-epoch second image center 18:51:23.549 -02:03:12.56
Angular distance between the image centers 0.01725 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_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits &> /tmp/tmp.KoZUDO1Hqs
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits &> /tmp/tmp.nVk6MgZYFx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits &> /tmp/tmp.WKcJ3AiKq8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits &> /tmp/tmp.XPC1RqyIWT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits and wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
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_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits and wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
Found non-empty wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits and wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
The reference image (wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits) and catalog (wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat) found
'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat' -> 'wcsmag.cat'
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
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 7408 out of 13310 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.858998
a=0.000000 b=1.000000 c=22.858998
From vast_summary.log: estimated ref. image limiting mag.: -8.06
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.80
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.80
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
2.3 pix Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
2.5 pix fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits
2.5 pix fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
Limiting magnitude estimates:
14.8 mag. Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
14.8 mag. Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
13.6 mag. fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits
13.6 mag. fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 10.9 (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.KoZUDO1Hqs (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_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits' -> 'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WCS-calibrated image found: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Checking if the catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WCS catalog name: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1253, passed=13310
Got 13310 stars (including 12037 good ones) from the SExtractor catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
util/solve_plate_with_UCAC5 got 13310 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (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...
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
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...
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits -region wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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.nVk6MgZYFx (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_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits' -> 'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WCS-calibrated image found: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
Checking if the catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WCS catalog name: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat
SExtractor catalog parsing summary: zero_flux=5, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1265, passed=13307
Got 13307 stars (including 12019 good ones) from the SExtractor catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat
util/solve_plate_with_UCAC5 got 13307 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (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...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits -region wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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.WKcJ3AiKq8 (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_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.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_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.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_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=306, passed=4406
Got 4406 stars (including 4096 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits.cat
util/solve_plate_with_UCAC5 got 4406 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...
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
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...
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.55"
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits -region wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.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.XPC1RqyIWT (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_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.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_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.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_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=323, passed=4513
Got 4513 stars (including 4185 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits.cat
util/solve_plate_with_UCAC5 got 4513 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...
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
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...
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.54"
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits -region wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits'
Saving fully-calibrated image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits'
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits'
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits'
Preparing the HTML report for the field Aql-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20855.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20855_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
Preparing report for the candidate 20855_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20871_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 20871_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 18:51:02.47 -06:14:10.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 11s
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 ####
18:51:04.31 -06:16:13.5
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_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
SExtractor catalog cache: saved Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat to cache
SExtractor catalog cache: saved Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Creating symlink local_wcs_cache/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.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_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits exists and is non-empty
wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits exists and is non-empty
wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits exists and is non-empty
wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:51:25.226 -01:59:55.32
Second-epoch image center 18:51:26.598 -02:02:30.53
Angular distance between the image centers 0.04 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:51:25.226 -01:59:55.32
Second-epoch image center 18:51:23.549 -02:03:12.56
Angular distance between the image centers 0.06 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 18:51:26.598 -02:02:30.53
Second-epoch second image center 18:51:23.549 -02:03:12.56
Angular distance between the image centers 0.01725 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_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits &> /tmp/tmp.6ybcbz37iK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits &> /tmp/tmp.2UAcSrTG3g
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits &> /tmp/tmp.ggnDlCg494
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits &> /tmp/tmp.WkNDghyqsa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits and wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
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_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits and wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
Found non-empty wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits and wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
The reference image (wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits) and catalog (wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat) found
'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat' -> 'wcsmag.cat'
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
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 8387 out of 153764 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.669636
a=0.000000 b=1.000000 c=22.669636
From vast_summary.log: estimated ref. image limiting mag.: -7.77
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.90
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.90
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 30 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
2.1 pix Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
2.3 pix fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits
2.2 pix fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
Limiting magnitude estimates:
14.9 mag. Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
14.9 mag. Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
13.7 mag. fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits
13.7 mag. fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 13.2 (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.6ybcbz37iK (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_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits' -> 'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WCS-calibrated image found: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Checking if the catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WCS catalog name: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=17867, passed=153743
Got 153743 stars (including 135593 good ones) from the SExtractor catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
util/solve_plate_with_UCAC5 got 153743 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (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...
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits -region wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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.2UAcSrTG3g (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_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits' -> 'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WCS-calibrated image found: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
Checking if the catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WCS catalog name: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=18180, passed=153307
Got 153307 stars (including 134827 good ones) from the SExtractor catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat
util/solve_plate_with_UCAC5 got 153307 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (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...
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
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...
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 941 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits -region wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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.ggnDlCg494 (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_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.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_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.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_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=2405, passed=50294
Got 50294 stars (including 47820 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits.cat
util/solve_plate_with_UCAC5 got 50294 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...
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...
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
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...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.53"
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits -region wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.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.WkNDghyqsa (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_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.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_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.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_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=2682, passed=51900
Got 51900 stars (including 49140 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits.cat
util/solve_plate_with_UCAC5 got 51900 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...
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
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...
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.51"
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 950 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits -region wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Saving fully-calibrated image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.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_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-17-39_20.00sec_-10.00C_LIGHT_0333.fits
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.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_2026-03-30_CI_Aql-03-Q2b1x1_041914_TTUQ2b1x1_19152_sIHCbHSj/wcs_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334.fits
Preparing the HTML report for the field Aql-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out178596.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178599.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178601.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178605.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178632.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178635.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178641.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178644.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178771.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178788.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178810.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out178640.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
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Considering the candidate 178596_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 178596_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 19:12:33.50 -00:17:17.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)
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Considering the candidate 178599_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 178599_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 19:09:12.61 +01:05:31.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 1.473 4267376086851487104 287.30263257867 +01.09248238766 12.8791 11.8508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.473#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 178601_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 178601_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 19:03:59.38 -02:13:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 2.377 4261795034539651584 285.99677630924 -02.23188510895 12.5999 11.4592 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.377#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 178605_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 178605_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 18:49:44.21 -06:19:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 2.682 4252507970869790464 282.43378395715 -06.32013593174 12.9811 12.5090 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.682#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 178612_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 178612_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 18:50:16.81 -00:13:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178615_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 178615_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 18:50:06.97 +01:20:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178617_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 178617_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 19:12:02.04 +00:53:32.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178620_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 178620_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 19:05:34.24 -00:25:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178621_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 178621_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 19:05:24.65 +01:48:23.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178622_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 178622_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 19:09:13.97 +01:18:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178632_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 178632_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 18:56:57.35 -04:25:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 0.814 4255354606471212416 284.23874231919 -04.41887573473 12.6892 11.9801 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.814#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 178635_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 178635_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 19:14:30.58 +00:04:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 1.214 4264022095326249728 288.62766136660 +00.08203744059 11.7939 10.5295 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.214#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 178640_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
Preparing report for the candidate 178640_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
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Considering the candidate 178641_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 178641_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 19:05:33.82 -00:03:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 3.247 4265666273197592832 286.39053532201 -00.06240499432 12.7152 11.8038 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.247#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 178644_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 178644_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 19:13:54.94 +01:29:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 2.071 4267736073816703872 288.47834266008 +01.49865166847 12.7361 12.0787 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.071#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 178646_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 178646_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 19:02:15.62 -01:01:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178648_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 178648_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 19:12:07.79 +02:09:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178650_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 178650_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 19:03:11.25 -00:26:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178677_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 178677_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 18:47:01.86 -04:44:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178692_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 178692_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 18:57:03.71 -05:49:03.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 178697_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 178697_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 19:04:20.73 -05:42:47.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 178702_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 178702_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 19:01:33.48 -05:43:08.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 178732_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 178732_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 19:02:58.77 -03:43:13.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 178771_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 178771_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 19:02:06.97 +01:26:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 0.876 4268294144642496640 285.52927291439 +01.43956318875 12.2026 11.1639 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.876#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 178788_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 178788_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 19:04:59.38 +01:36:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 3.868 4267576575886742016 286.24635554670 +01.60235569760 12.9949 12.5413 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.868#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 178810_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 178810_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 18:45:03.91 -05:29:21.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 2.353 4253542302077944704 281.26587500928 -05.48871707273 12.5588 11.5201 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.353#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 178813_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 178813_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 18:56:56.89 -00:47:05.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178847_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 178847_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 18:56:11.28 -00:29:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84001_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 84001_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks
**** FOUND 18:58:41.82 -02:20:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 135709_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334
The candidate 135709_fd_Aql-03-Q2b1x1_2026-03-30_04-18-34_20.00sec_-10.00C_LIGHT_0334 did not pass the final checks