This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
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
target,2461124.9893,13.71,0.05,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
target 20260325.4893 13.71CV 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/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:28:00.81 +79:01:40.3 ;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_Cep-02-Q2b1x1_2025-12-26_20-12-22_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20_00sec_-15_00C_LIGHT_0223_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20_00sec_-15_00C_LIGHT_0223_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
NSVS J2344541+782022,2461124.9893,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2344541+782022 20260325.4893 12.98CV 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/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:44:54.81 +78:20:20.7 ;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_Cep-02-Q2b1x1_2025-12-26_20-12-22_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20_00sec_-15_00C_LIGHT_0223_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png resample_wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20_00sec_-15_00C_LIGHT_0223_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: 2461036.59203935 27.12.2025 02:12:22.200 /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
First image: 2461036.59203935 27.12.2025 02:12:22.200 /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
Last image: 2461124.98952742 25.03.2026 11:44:45.169 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.90
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: 5 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): 12518
Objects passed selection criteria: 12437
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 7818.75
Average stars matched: 7455.75 (95.3573 %)
Memory usage VmPeak: 118020 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 Wed Mar 25 06:48:23 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: 2461036.59203935 27.12.2025 02:12:22.200 /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
First image: 2461036.59203935 27.12.2025 02:12:22.200 /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
Last image: 2461124.98952742 25.03.2026 11:44:45.169 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 57
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.56
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: 45 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): 84911
Objects passed selection criteria: 84659
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 57924.8
Average stars matched: 54737.8 (94.498 %)
Memory usage VmPeak: 1990028 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 Wed Mar 25 06:50:23 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/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
SExtractor catalog cache: saved Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits.cat to cache
SExtractor catalog cache: saved Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.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/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.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: 2461124.98900650
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_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits exists and is non-empty
Saving wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits to local_wcs_cache/
'wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits' -> 'local_wcs_cache/wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits'
wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits exists and is non-empty
Saving wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits to local_wcs_cache/
'wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits' -> 'local_wcs_cache/wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits'
wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits exists and is non-empty
Saving wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits to local_wcs_cache/
'wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits' -> 'local_wcs_cache/wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits'
wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits exists and is non-empty
Saving wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits to local_wcs_cache/
'wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits' -> 'local_wcs_cache/wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.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 00:00:08.538 +77:29:46.61
Second-epoch image center 00:00:03.471 +77:29:55.86
Angular distance between the image centers 0.01 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 00:00:08.538 +77:29:46.61
Second-epoch image center 00:00:03.497 +77:29:47.39
Angular distance between the image centers 0.00 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 00:00:03.471 +77:29:55.86
Second-epoch second image center 00:00:03.497 +77:29:47.39
Angular distance between the image centers 0.00235 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/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits &> /tmp/tmp.JkjjsAngfg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits &> /tmp/tmp.ZqiMtsGt9q
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits &> /tmp/tmp.8F7DprEBCM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits &> /tmp/tmp.21RA6KubIK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
Calibrating the magnitude scale
Found non-empty wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.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_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.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_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits.cat
Found non-empty wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits.cat
The reference image (wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits) and catalog (wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits.cat) found
'wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.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 8943 out of 14293 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.920108
a=0.000000 b=1.000000 c=22.920108
From vast_summary.log: estimated ref. image limiting mag.: -7.90
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.02
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.02
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
2.5 pix Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits
2.3 pix fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits
2.3 pix fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
Limiting magnitude estimates:
15.0 mag. Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
15.0 mag. Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits
13.4 mag. fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits
13.4 mag. fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
All-image limiting magnitude estimate: 13.4 (SNR ) 10.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.JkjjsAngfg (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/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.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_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits' -> 'wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
WCS_IMAGE_NAME=wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
WCS-calibrated image found: wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
Checking if the catalog wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits.cat corresponding to the image wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits alredy exist and is non-empty...
Catalog wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits.cat corresponding to the image wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
WCS catalog name: wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1285, passed=14293
Got 14293 stars (including 12992 good ones) from the SExtractor catalog wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits.cat
util/solve_plate_with_UCAC5 got 14293 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 975 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: 0.45"
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 975 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: 0.43"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits -region wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.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.ZqiMtsGt9q (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/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.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_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits' -> 'wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits
WCS_IMAGE_NAME=wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits
WCS-calibrated image found: wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits
Checking if the catalog wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits.cat corresponding to the image wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits alredy exist and is non-empty...
Catalog wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits.cat corresponding to the image wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits
WCS catalog name: wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1272, passed=14344
Got 14344 stars (including 13060 good ones) from the SExtractor catalog wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits.cat
util/solve_plate_with_UCAC5 got 14344 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 973 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 973 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: 0.42"
Excluding outliers - 971 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits -region wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.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.8F7DprEBCM (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_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.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_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits
WCS_IMAGE_NAME=wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits
WCS-calibrated image found: wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits
Checking if the catalog wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits.cat corresponding to the image wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits.cat corresponding to the image wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits
WCS catalog name: wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=186, passed=3368
Got 3368 stars (including 3178 good ones) from the SExtractor catalog wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits.cat
util/solve_plate_with_UCAC5 got 3368 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 963 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 963 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: 0.43"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits -region wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.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.21RA6KubIK (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_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.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_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
WCS_IMAGE_NAME=wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
WCS-calibrated image found: wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
Checking if the catalog wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits.cat corresponding to the image wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits.cat corresponding to the image wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
WCS catalog name: wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=178, passed=3141
Got 3141 stars (including 2960 good ones) from the SExtractor catalog wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits.cat
util/solve_plate_with_UCAC5 got 3141 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 963 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: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.46"
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits -region wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.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_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits'
Saving fully-calibrated image wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits'
Saving fully-calibrated image wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits'
Saving fully-calibrated image wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits'
Preparing the HTML report for the field Cep-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
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 02399_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 02399_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 00:38:22.73 +80:21:24.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Cep-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
SExtractor catalog cache: saved Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits.cat to cache
SExtractor catalog cache: saved Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
Creating symlink local_wcs_cache/wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits
Creating symlink local_wcs_cache/wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits
Creating symlink local_wcs_cache/wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.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_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits exists and is non-empty
wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits exists and is non-empty
wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits exists and is non-empty
wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.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 00:00:08.538 +77:29:46.61
Second-epoch image center 00:00:03.471 +77:29:55.86
Angular distance between the image centers 0.01 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 00:00:08.538 +77:29:46.61
Second-epoch image center 00:00:03.497 +77:29:47.39
Angular distance between the image centers 0.00 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 00:00:03.471 +77:29:55.86
Second-epoch second image center 00:00:03.497 +77:29:47.39
Angular distance between the image centers 0.00235 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/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits &> /tmp/tmp.nFwhPkVqtd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits &> /tmp/tmp.1gaUe0QyPt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits &> /tmp/tmp.AWlosWXGDy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits &> /tmp/tmp.O8ONrm4k3k
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
Calibrating the magnitude scale
Found non-empty wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.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_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.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_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits.cat
Found non-empty wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits.cat
The reference image (wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits) and catalog (wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits.cat) found
'wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.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 9294 out of 99240 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.753855
a=0.000000 b=1.000000 c=22.753855
From vast_summary.log: estimated ref. image limiting mag.: -7.56
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.19
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.19
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 47 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
2.2 pix Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits
2.1 pix fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits
2.1 pix fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
Limiting magnitude estimates:
15.2 mag. Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
15.2 mag. Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits
13.7 mag. fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits
13.7 mag. fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 13.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.nFwhPkVqtd (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/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.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_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits' -> 'wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
WCS_IMAGE_NAME=wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
WCS-calibrated image found: wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
Checking if the catalog wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits.cat corresponding to the image wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits alredy exist and is non-empty...
Catalog wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits.cat corresponding to the image wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
WCS catalog name: wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=31, blended=9268, passed=99209
Got 99209 stars (including 89782 good ones) from the SExtractor catalog wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits.cat
util/solve_plate_with_UCAC5 got 99209 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 974 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: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
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 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits -region wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.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.1gaUe0QyPt (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/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.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_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits' -> 'wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits
WCS_IMAGE_NAME=wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits
WCS-calibrated image found: wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits
Checking if the catalog wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits.cat corresponding to the image wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits alredy exist and is non-empty...
Catalog wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits.cat corresponding to the image wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits
WCS catalog name: wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=30, blended=9278, passed=98051
Got 98051 stars (including 88613 good ones) from the SExtractor catalog wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits.cat
util/solve_plate_with_UCAC5 got 98051 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 973 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: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
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 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits -region wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.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.AWlosWXGDy (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_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.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_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits
WCS_IMAGE_NAME=wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits
WCS-calibrated image found: wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits
Checking if the catalog wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits.cat corresponding to the image wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits.cat corresponding to the image wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits
WCS catalog name: wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=998, passed=28885
Got 28885 stars (including 27842 good ones) from the SExtractor catalog wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits.cat
util/solve_plate_with_UCAC5 got 28885 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 963 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 963 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: 0.41"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits -region wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.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.O8ONrm4k3k (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_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.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_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
WCS_IMAGE_NAME=wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
WCS-calibrated image found: wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
Checking if the catalog wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits.cat corresponding to the image wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits.cat corresponding to the image wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
WCS catalog name: wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=920, passed=28140
Got 28140 stars (including 27177 good ones) from the SExtractor catalog wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits.cat
util/solve_plate_with_UCAC5 got 28140 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 964 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: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits -region wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.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_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.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_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/wcs_Cep-02-Q2b1x1_2025-12-26_20-12-22_20.00sec_-15.00C_LIGHT_0067.fits
Saving fully-calibrated image wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.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_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/wcs_Cep-02-Q2b1x1_2025-12-26_20-12-59_20.00sec_-15.00C_LIGHT_0068.fits
Saving fully-calibrated image wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.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_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-00_20.00sec_-15.00C_LIGHT_0223.fits
Saving fully-calibrated image wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.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_2026-03-25_CI_Cep-02-Q2b1x1_064602_TTUQ2b1x1_22825_ltd6wyFP/wcs_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224.fits
Preparing the HTML report for the field Cep-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out116640.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116644.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116646.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116648.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116652.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116653.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116655.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116656.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117617.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118439.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118455.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out119325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out119508.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out119511.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out119846.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out119937.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out119979.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out120046.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out120111.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out120217.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out120319.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out120702.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out120732.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out120905.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out121215.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out121471.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37160.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 20s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 116635_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 116635_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 23:39:46.73 +76:57:22.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116640_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 116640_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 23:17:07.75 +76:53:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 1.096 2281264427505973760 349.28097465480 +76.88827428998 13.6207 13.0508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.096#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116641_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 116641_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 23:22:30.47 +76:38:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116644_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 116644_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 23:16:32.17 +78:36:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 1.982 2282781478672988160 349.13143802877 +78.61038632867 13.4904 12.9296 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.982#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116646_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 116646_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 22:26:59.23 +74:25:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 1.725 2279437142258610944 336.74766620183 +74.43127869111 13.4863 12.8601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.725#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116647_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 116647_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 22:56:51.09 +74:34:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116648_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 116648_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 22:50:02.11 +75:34:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 2.125 2281080053149298432 342.50851736332 +75.57700293661 13.2262 12.3295 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.125#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116652_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 116652_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 23:26:06.36 +78:06:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 0.908 2281947258585639552 351.52589531448 +78.11460832533 13.1631 12.6806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.908#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116653_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 116653_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 23:05:45.99 +76:09:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 0.475 2233177492622850176 346.44216786182 +76.15664313933 13.3639 12.8315 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.475#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116655_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 116655_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 23:12:23.28 +78:16:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 0.279 2282387406834356480 348.09687849160 +78.27031542781 12.7913 12.2824 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.279#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116656_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 116656_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 00:00:21.39 +79:24:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 1.389 564627193987382400 000.08999551301 +79.40534323148 12.7158 11.9220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.389#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117617_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 117617_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 23:08:28.42 +75:22:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)GAIADR2_OUTPUT=# 0.227 2232895124292808960 347.11865185443 +75.38306185432 11.5619 11.1024 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.227#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118286_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 118286_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 01:19:42.23 +80:52:35.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118439_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 118439_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 23:06:22.63 +75:33:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.541 2233088049927908992 346.59371276682 +75.55976356689 11.9228 10.9758 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.541#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118455_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 118455_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 00:13:34.30 +76:01:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 0.920 539783316442499328 003.39191044884 +76.01803235120 11.7712 11.2575 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.920#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118569_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 118569_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 119260_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 119260_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 00:47:25.16 +74:51:53.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 119325_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 119325_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 23:20:00.38 +73:55:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 0.877 2231780455722894336 350.00223479845 +73.92502485024 12.6957 12.0053 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.877#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 119507_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 119507_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 119508_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 119508_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 00:43:00.19 +76:58:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 1.704 563333274960162816 010.74963847990 +76.97857662032 12.2755 11.7477 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.704#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 119511_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 119511_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 23:04:09.81 +74:27:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)GAIADR2_OUTPUT=# 1.486 2232698655309571328 346.03942080832 +74.45538584060 13.1233 12.5101 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.486#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 119670_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 119670_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 00:01:40.25 +73:38:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 119846_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 119846_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 23:49:06.61 +78:51:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 0.831 2282099540945825920 357.27637479566 +78.85627143246 13.0055 12.1644 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.831#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 119937_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 119937_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 23:55:04.10 +76:58:24.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 0.502 2233430345937980160 358.76647807707 +76.97350096751 13.0321 12.4292 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.502#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 119979_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 119979_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 00:32:30.75 +76:33:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 0.986 540037471129091968 008.12698366177 +76.55467886236 12.0079 11.1531 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.986#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 120046_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 120046_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 00:03:02.09 +76:18:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 1.305 539829083614248064 000.75750951323 +76.31678146180 12.6467 12.0280 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.305#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 120111_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 120111_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 00:20:32.51 +76:34:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 1.219 540000607426851712 005.13537972154 +76.58297694422 12.5305 11.8935 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.219#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 120151_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 120151_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 23:28:32.78 +76:22:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120217_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 120217_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 00:14:13.20 +76:03:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 0.502 539772183887256832 003.55500457826 +76.06152840693 12.1939 11.2582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.502#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 120319_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 120319_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 22:37:36.67 +76:44:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 3.420 2280696048712989824 339.40597230642 +76.74705344867 13.5667 13.0840 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 120488_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 120488_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 120598_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 120598_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 120702_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 120702_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 23:20:42.86 +77:39:34.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 2.503 2281732304062877696 350.18179451436 +77.65936039253 13.6408 13.1010 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.503#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 120732_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 120732_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 23:55:16.85 +74:51:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 1.281 2229250964802128000 358.81949466276 +74.85302535565 12.9631 12.3256 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.281#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 120738_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 120738_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 120905_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 120905_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 22:54:24.68 +74:33:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 2.592 2232749885679022080 343.60492541145 +74.55642818853 13.5084 13.0934 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.592#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 121167_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 121167_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 121202_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 121202_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 121215_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 121215_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 22:57:23.71 +77:37:02.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 1.057 2282340299632656768 344.34990676541 +77.61755937000 13.5055 13.0040 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.057#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 121429_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 121429_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 121471_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
Preparing report for the candidate 121471_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
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Considering the candidate 98730_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 98730_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52620_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 52620_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 85417_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 85417_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 00:13:10.37 +73:51:47.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13609_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 13609_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks
**** FOUND 00:38:22.79 +80:21:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92288_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224
The candidate 92288_fd_Cep-02-Q2b1x1_2026-03-25_06-44-45_20.00sec_-14.90C_LIGHT_0224 did not pass the final checks