This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 03 25.4934 2461124.9934 13.02 19:42:26.78 +60:39:46.4
92.85623 17.53298 galactic Dra Second-epoch detections are separated by 6.1" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J295.6071+60.6618 | 19:42:26.78 +60:39:46.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J295.6071+60.6618,2461124.9934,13.02,0.05,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
ATO J295.6071+60.6618 20260325.4934 13.02CV 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-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:42:26.78 +60:39:46.4 ;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-05-Q2b1x1_2026-03-19_06-59-47_20_00sec_-15_00C_LIGHT_0233_fits__*pix.png resample_wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20_00sec_-15_00C_LIGHT_0230_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20_00sec_-15_00C_LIGHT_0233_fits__*pix.png resample_wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20_00sec_-14_90C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20_00sec_-15_00C_LIGHT_0233_fits__*pix.png resample_wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20_00sec_-15_00C_LIGHT_0230_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20_00sec_-15_00C_LIGHT_0233_fits__*pix.png resample_wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20_00sec_-14_90C_LIGHT_0229_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 3200728,2461124.9934,12.85,0.05,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 3200728 20260325.4934 12.85CV 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-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:44:34.11 +63:01:57.2 ;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-05-Q2b1x1_2026-03-19_06-59-47_20_00sec_-15_00C_LIGHT_0233_fits__*pix.png resample_wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20_00sec_-15_00C_LIGHT_0230_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20_00sec_-15_00C_LIGHT_0233_fits__*pix.png resample_wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20_00sec_-14_90C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20_00sec_-15_00C_LIGHT_0233_fits__*pix.png resample_wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20_00sec_-15_00C_LIGHT_0230_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20_00sec_-15_00C_LIGHT_0233_fits__*pix.png resample_wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20_00sec_-14_90C_LIGHT_0229_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: 2461118.99997240 19.03.2026 11:59:47.615 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
First image: 2461118.99997240 19.03.2026 11:59:47.615 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
Last image: 2461124.99372299 25.03.2026 11:50:47.666 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.44
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 8921
Objects passed selection criteria: 8909
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 7463.5
Average stars matched: 7359.5 (98.6066 %)
Memory usage VmPeak: 115548 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 06:54:20 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: 2461118.99997240 19.03.2026 11:59:47.615 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
First image: 2461118.99997240 19.03.2026 11:59:47.615 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
Last image: 2461124.99372299 25.03.2026 11:50:47.666 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 60
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.09
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: 34 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): 68360
Objects passed selection criteria: 68232
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 60504.5
Average stars matched: 59014.8 (97.5378 %)
Memory usage VmPeak: 1858884 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 06:55:37 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-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits
SExtractor catalog cache: saved Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits.cat to cache
SExtractor catalog cache: saved Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.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-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.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: 2461124.99315561
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-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits exists and is non-empty
Saving wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits to local_wcs_cache/
'wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits' -> 'local_wcs_cache/wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits'
wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits exists and is non-empty
Saving wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits to local_wcs_cache/
'wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits' -> 'local_wcs_cache/wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits'
wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits exists and is non-empty
Saving wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits to local_wcs_cache/
'wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits' -> 'local_wcs_cache/wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits'
wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits exists and is non-empty
Saving wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits to local_wcs_cache/
'wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits' -> 'local_wcs_cache/wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits'
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 20:34:18.899 +62:00:06.79
Second-epoch image center 20:34:18.490 +61:59:50.92
Angular distance between the image centers 0.00 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 20:34:18.899 +62:00:06.79
Second-epoch image center 20:34:19.417 +62:00:27.24
Angular distance between the image centers 0.01 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 20:34:18.490 +61:59:50.92
Second-epoch second image center 20:34:19.417 +62:00:27.24
Angular distance between the image centers 0.01025 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-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits &> /tmp/tmp.Gg0Obnu8qh
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits &> /tmp/tmp.sQxzS5GZyF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits &> /tmp/tmp.mCowQWwdwL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits &> /tmp/tmp.xA3s6Pwz4w
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits
Calibrating the magnitude scale
Found non-empty wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.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-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits and wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.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-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits and wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits.cat
Found non-empty wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits and wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits.cat
The reference image (wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits) and catalog (wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits.cat) found
'wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.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 9043 out of 11818 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.916433
a=0.000000 b=1.000000 c=22.916433
From vast_summary.log: estimated ref. image limiting mag.: -8.44
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.48
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.48
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
2.4 pix Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits
2.4 pix fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits
2.4 pix fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits
Limiting magnitude estimates:
14.5 mag. Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
14.4 mag. Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits
13.7 mag. fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits
13.7 mag. fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 10.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Gg0Obnu8qh (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.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-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits' -> 'wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
WCS_IMAGE_NAME=wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
WCS-calibrated image found: wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
Checking if the catalog wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits.cat corresponding to the image wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits alredy exist and is non-empty...
Catalog wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits.cat corresponding to the image wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
WCS catalog name: wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=996, passed=11818
Got 11818 stars (including 10804 good ones) from the SExtractor catalog wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits.cat
util/solve_plate_with_UCAC5 got 11818 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 972 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: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.54"
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits -region wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.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.sQxzS5GZyF (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.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-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits' -> 'wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits
WCS_IMAGE_NAME=wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits
WCS-calibrated image found: wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits
Checking if the catalog wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits.cat corresponding to the image wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits alredy exist and is non-empty...
Catalog wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits.cat corresponding to the image wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits
WCS catalog name: wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=975, passed=11288
Got 11288 stars (including 10298 good ones) from the SExtractor catalog wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits.cat
util/solve_plate_with_UCAC5 got 11288 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 970 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: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.57"
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits -region wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.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.mCowQWwdwL (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-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.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-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits
WCS_IMAGE_NAME=wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits
WCS-calibrated image found: wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits
Checking if the catalog wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits.cat corresponding to the image wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits.cat corresponding to the image wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.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-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits
WCS catalog name: wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=409, passed=6631
Got 6631 stars (including 6215 good ones) from the SExtractor catalog wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits.cat
util/solve_plate_with_UCAC5 got 6631 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 969 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: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.53"
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits -region wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.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.xA3s6Pwz4w (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-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.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-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits
WCS_IMAGE_NAME=wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits
WCS-calibrated image found: wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits
Checking if the catalog wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits.cat corresponding to the image wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits.cat corresponding to the image wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.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-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits
WCS catalog name: wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=415, passed=6498
Got 6498 stars (including 6076 good ones) from the SExtractor catalog wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits.cat
util/solve_plate_with_UCAC5 got 6498 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
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 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.55"
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits -region wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.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-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits'
Saving fully-calibrated image wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits'
Saving fully-calibrated image wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits'
Saving fully-calibrated image wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits'
Preparing the HTML report for the field Cep-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Cep-05-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-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits
SExtractor catalog cache: saved Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits.cat to cache
SExtractor catalog cache: saved Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.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-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
Creating symlink local_wcs_cache/wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits
Creating symlink local_wcs_cache/wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits
Creating symlink local_wcs_cache/wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.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-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits exists and is non-empty
wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits exists and is non-empty
wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits exists and is non-empty
wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits exists and is non-empty
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 20:34:18.899 +62:00:06.79
Second-epoch image center 20:34:18.490 +61:59:50.92
Angular distance between the image centers 0.00 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 20:34:18.899 +62:00:06.79
Second-epoch image center 20:34:19.417 +62:00:27.24
Angular distance between the image centers 0.01 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 20:34:18.490 +61:59:50.92
Second-epoch second image center 20:34:19.417 +62:00:27.24
Angular distance between the image centers 0.01025 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-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits &> /tmp/tmp.UBxqOB8eTX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits &> /tmp/tmp.fwx1LNcptP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits &> /tmp/tmp.d2CqdqajZO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits &> /tmp/tmp.rijBtB1HGi
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits
Calibrating the magnitude scale
Found non-empty wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.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-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits and wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.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-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits and wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits.cat
Found non-empty wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits and wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits.cat
The reference image (wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits) and catalog (wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits.cat) found
'wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.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 11566 out of 85855 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.712373
a=0.000000 b=1.000000 c=22.712373
From vast_summary.log: estimated ref. image limiting mag.: -8.09
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.62
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.62
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 50 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
2.2 pix Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits
2.2 pix fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits
2.2 pix fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits
Limiting magnitude estimates:
14.6 mag. Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
14.6 mag. Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits
13.9 mag. fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits
13.9 mag. fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 13.4 (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.UBxqOB8eTX (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.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-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits' -> 'wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
WCS_IMAGE_NAME=wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
WCS-calibrated image found: wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
Checking if the catalog wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits.cat corresponding to the image wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits alredy exist and is non-empty...
Catalog wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits.cat corresponding to the image wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
WCS catalog name: wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=6148, passed=85835
Got 85835 stars (including 79584 good ones) from the SExtractor catalog wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits.cat
util/solve_plate_with_UCAC5 got 85835 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 971 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: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.54"
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits -region wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.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.fwx1LNcptP (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.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-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits' -> 'wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits
WCS_IMAGE_NAME=wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits
WCS-calibrated image found: wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits
Checking if the catalog wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits.cat corresponding to the image wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits alredy exist and is non-empty...
Catalog wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits.cat corresponding to the image wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits
WCS catalog name: wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=26, blended=5705, passed=83112
Got 83112 stars (including 77292 good ones) from the SExtractor catalog wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits.cat
util/solve_plate_with_UCAC5 got 83112 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 970 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: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.56"
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits -region wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.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.d2CqdqajZO (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-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.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-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits
WCS_IMAGE_NAME=wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits
WCS-calibrated image found: wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits
Checking if the catalog wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits.cat corresponding to the image wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits.cat corresponding to the image wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.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-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits
WCS catalog name: wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=2497, passed=53489
Got 53489 stars (including 50910 good ones) from the SExtractor catalog wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits.cat
util/solve_plate_with_UCAC5 got 53489 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
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 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.52"
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 966 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits -region wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.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.rijBtB1HGi (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-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.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-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits
WCS_IMAGE_NAME=wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits
WCS-calibrated image found: wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits
Checking if the catalog wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits.cat corresponding to the image wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits.cat corresponding to the image wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.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-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits
WCS catalog name: wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=7, blended=2434, passed=52759
Got 52759 stars (including 50258 good ones) from the SExtractor catalog wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits.cat
util/solve_plate_with_UCAC5 got 52759 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.52"
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cep-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits -region wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.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-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.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-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits
Saving fully-calibrated image wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.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-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/wcs_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits
Saving fully-calibrated image wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.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-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-49-58_20.00sec_-14.90C_LIGHT_0229.fits
Saving fully-calibrated image wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.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-05-Q2b1x1_065207_TTUQ2b1x1_31625_YIVMXdLH/wcs_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230.fits
Preparing the HTML report for the field Cep-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out101212.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101216.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101219.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101221.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101223.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101224.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101225.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101229.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101230.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101233.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101234.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101238.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101245.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101328.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101398.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101411.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101447.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101456.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101478.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101485.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101490.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101494.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101499.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101507.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101511.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101515.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101517.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101524.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101532.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101545.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101564.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101565.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101572.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101618.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101625.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101643.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out101228.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67542.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 12s
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 101212_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101212_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:26:38.49 +60:32:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.918 2194759422479670400 306.66101182519 +60.54501354649 13.7021 13.0964 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.918#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101216_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101216_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:19:44.42 +62:17:42.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)
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Considering the candidate 101219_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101219_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:59:58.78 +61:12:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 0.847 2195610440179597056 314.99462687249 +61.21078278897 12.7769 11.5624 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.847#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101221_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101221_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:05:35.57 +61:12:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 0.811 2237785511496607360 301.39856806539 +61.21466131806 13.6079 13.0298 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.811#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101223_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101223_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:07:22.74 +61:59:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 1.479 2237950060284046976 301.84560835761 +61.99872498494 13.0917 12.6817 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.479#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101224_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101224_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 19:36:19.24 +64:05:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 3.869 2242310208002380416 294.07770723846 +64.09064499067 13.2846 12.8679 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.869#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101225_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101225_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:10:41.47 +65:47:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 0.548 2248001177107699456 302.67299962685 +65.78451496480 13.2514 12.7049 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.548#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101228_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
Preparing report for the candidate 101228_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
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Considering the candidate 101229_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101229_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 21:03:24.24 +64:48:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 0.170 2197408833183603840 315.85088885233 +64.80083436973 12.8365 12.1440 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.170#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101230_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101230_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:52:40.44 +59:13:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 0.438 2193825799668373888 313.16829408125 +59.22677223113 12.8639 12.1549 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.438#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101233_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101233_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:41:26.49 +63:05:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 0.836 2195485031434107392 310.36017634721 +63.08663066608 12.8091 12.0658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.836#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101234_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101234_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 19:47:10.38 +59:02:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.308 2235862289562487040 296.79290781844 +59.03990116310 12.9645 12.5106 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.308#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101238_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101238_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:18:11.76 +61:30:12.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)
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Considering the candidate 101241_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101241_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:23:48.85 +63:33:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101242_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101242_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:13:29.80 +66:06:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101245_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101245_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 19:59:29.16 +60:05:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 0.490 2237281454134294784 299.87160452122 +60.09926466233 11.7685 11.0438 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.490#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101328_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101328_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:17:52.86 +59:48:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.75, MAG_FAINT_SEARCH_LIMIT=12.73)GAIADR2_OUTPUT=# 4.161 2236663356801894400 304.46973095830 +59.80593160712 12.0374 11.2953 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.161#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101397_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101397_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 19:47:26.67 +64:31:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101398_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101398_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 21:06:11.39 +62:55:25.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 2.009 2196358245526059136 316.54866866253 +62.92392152805 12.6491 11.9523 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.009#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101408_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101408_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 19:39:25.67 +65:22:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101411_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101411_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:21:26.60 +63:27:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 0.626 2243728681081901952 305.36073348470 +63.45722365285 12.2998 11.4391 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.626#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101447_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101447_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 21:12:48.63 +60:07:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 2.017 2192289816285682176 318.20281307763 +60.13185803690 12.4768 11.8014 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.017#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101456_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101456_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:28:05.96 +59:44:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 0.710 2188659675566064512 307.02518680401 +59.74514034007 12.6775 11.8158 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.710#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101467_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101467_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:35:12.56 +62:27:08.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 2.050 2195359996346594816 308.80309767248 +62.45194256992 13.0101 12.0876 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.050#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101478_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101478_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:07:51.68 +64:19:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 2.011 2244450819703096832 301.96428096562 +64.32276719263 13.0865 12.5380 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.011#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101485_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101485_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:21:20.22 +64:42:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 3.416 2244694876924753792 305.33243681656 +64.70663130647 12.7529 11.7639 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.416#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101490_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101490_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 19:40:21.13 +63:50:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 2.139 2242242244439870208 295.08867345705 +63.84339169998 13.1744 12.6835 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.139#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101492_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101492_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:55:19.75 +65:41:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101493_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101493_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:05:21.14 +62:00:43.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 101494_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101494_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:26:33.00 +60:32:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 2.681 2194757945010919424 306.63680001885 +60.55043821083 13.3063 12.7307 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.681#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101499_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101499_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:29:23.02 +60:26:06.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)
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Considering the candidate 101507_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101507_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 19:57:59.63 +64:00:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 1.091 2247328275992580608 299.49777516223 +64.01393573097 13.3218 12.7901 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.091#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101511_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101511_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:30:41.20 +58:17:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 4.403 2188328993144793472 307.67351317205 +58.29710542763 13.1170 12.5789 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.403#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101515_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101515_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 21:20:41.43 +62:31:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 1.040 2193153345230109696 320.17292431880 +62.52691305208 13.0113 12.5331 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.040#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101517_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101517_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:35:28.36 +58:07:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 1.442 2187540372729109632 308.86741173843 +58.11868298102 13.2432 12.7560 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.442#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101524_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101524_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:57:48.85 +61:21:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 0.638 2195603465152704256 314.45329941416 +61.35196701375 12.8068 11.9924 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.638#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101532_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101532_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:12:41.04 +64:52:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 4.518 2244796856628242560 303.16908669048 +64.86726577065 13.5262 12.9912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.518#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101545_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101545_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:08:46.98 +62:04:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 0.754 2237927898253004160 302.19577797086 +62.07176469983 13.1072 12.6148 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.754#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101564_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101564_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:15:44.41 +61:29:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 2.806 2237092235056375168 303.93350187392 +61.49873198277 13.3217 12.6881 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.806#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101565_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101565_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:35:15.79 +61:48:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 2.925 2195302924820554240 308.81655996916 +61.81714375672 13.2697 12.4003 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.925#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101572_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101572_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:01:30.39 +62:23:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.599 2238173158064630528 300.37591862815 +62.39661643037 13.3030 12.8228 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.599#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101579_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101579_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:26:40.27 +58:47:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101589_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101589_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 19:34:09.74 +63:51:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101594_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101594_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:35:11.14 +62:26:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 3.342 2195359961986856576 308.79663813506 +62.44704949862 13.5138 12.7429 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.342#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101618_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101618_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:11:24.91 +65:03:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 1.389 2244849427028048640 302.85293664090 +65.05260925819 13.6695 13.0885 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 101619_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101619_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:51:36.47 +66:01:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 2.401 2245677496722377472 312.90273637566 +66.02382953072 13.2802 12.4635 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101625_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101625_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 19:52:31.11 +64:09:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 0.280 2241572470060350336 298.12966917751 +64.15788090031 13.5088 12.7003 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.280#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101634_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101634_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks
**** FOUND 20:03:19.72 +65:04:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101643_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230
The candidate 101643_fd_Cep-05-Q2b1x1_2026-03-25_06-50-47_20.00sec_-15.00C_LIGHT_0230 did not pass the final checks