This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9748,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4748 13.65CV 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/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:51:55.89 +71:30:02.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20_00sec_-14_90C_LIGHT_0526_fits__*pix.png resample_wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20_00sec_-14_90C_LIGHT_0202_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20_00sec_-14_90C_LIGHT_0526_fits__*pix.png resample_wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20_00sec_-15_00C_LIGHT_0201_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20_00sec_-14_90C_LIGHT_0526_fits__*pix.png resample_wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20_00sec_-14_90C_LIGHT_0202_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20_00sec_-14_90C_LIGHT_0526_fits__*pix.png resample_wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20_00sec_-15_00C_LIGHT_0201_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!
TCP 2026 03 25.4748* 10 48 58.27 +70 06 55.3 13.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9748,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4748 13.14CV 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/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:48:58.27 +70:06:55.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20_00sec_-14_90C_LIGHT_0526_fits__*pix.png resample_wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20_00sec_-14_90C_LIGHT_0202_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20_00sec_-14_90C_LIGHT_0526_fits__*pix.png resample_wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20_00sec_-15_00C_LIGHT_0201_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20_00sec_-14_90C_LIGHT_0526_fits__*pix.png resample_wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20_00sec_-14_90C_LIGHT_0202_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20_00sec_-14_90C_LIGHT_0526_fits__*pix.png resample_wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20_00sec_-15_00C_LIGHT_0201_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
target,2461124.9748,13.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4748 13.99CV 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/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:01:17.75 +69:56:33.9 ;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_Dra-03-Q2b1x1_2026-01-21_04-56-46_20_00sec_-14_90C_LIGHT_0526_fits__*pix.png resample_wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20_00sec_-14_90C_LIGHT_0202_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20_00sec_-14_90C_LIGHT_0526_fits__*pix.png resample_wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20_00sec_-15_00C_LIGHT_0201_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20_00sec_-14_90C_LIGHT_0526_fits__*pix.png resample_wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20_00sec_-14_90C_LIGHT_0202_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20_00sec_-14_90C_LIGHT_0526_fits__*pix.png resample_wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20_00sec_-15_00C_LIGHT_0201_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: 2461061.95621185 21.01.2026 10:56:46.704 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
First image: 2461061.95621185 21.01.2026 10:56:46.704 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
Last image: 2461124.97501066 25.03.2026 11:23:50.921 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
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): 6495
Objects passed selection criteria: 6462
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 4469.25
Average stars matched: 4358.75 (97.5275 %)
Memory usage VmPeak: 112960 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 06:26:13 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: 2461061.95621185 21.01.2026 10:56:46.704 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
First image: 2461061.95621185 21.01.2026 10:56:46.704 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
Last image: 2461124.97501066 25.03.2026 11:23:50.921 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 68
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.35
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: 12 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): 33243
Objects passed selection criteria: 33171
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 25169.8
Average stars matched: 24220 (96.2266 %)
Memory usage VmPeak: 137260 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 06:26:53 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/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits
SExtractor catalog cache: saved Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits.cat to cache
SExtractor catalog cache: saved Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.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/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.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: 2461124.97451588
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_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits exists and is non-empty
Saving wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits to local_wcs_cache/
'wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits' -> 'local_wcs_cache/wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits'
wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits exists and is non-empty
Saving wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits to local_wcs_cache/
'wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits' -> 'local_wcs_cache/wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits'
wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits exists and is non-empty
Saving wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits to local_wcs_cache/
'wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits' -> 'local_wcs_cache/wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits'
wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits exists and is non-empty
Saving wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits to local_wcs_cache/
'wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits' -> 'local_wcs_cache/wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 12:00:25.175 +69:59:06.47
Second-epoch image center 12:00:01.978 +69:59:51.64
Angular distance between the image centers 0.04 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 12:00:25.175 +69:59:06.47
Second-epoch image center 12:00:01.602 +69:59:54.16
Angular distance between the image centers 0.04 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 12:00:01.978 +69:59:51.64
Second-epoch second image center 12:00:01.602 +69:59:54.16
Angular distance between the image centers 0.00088 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00088 deg. (min. required shift: 0.00164 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/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits &> /tmp/tmp.2Re6C0HO45
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits &> /tmp/tmp.6MhyLdEsOH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits &> /tmp/tmp.gJfzt1hovk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits &> /tmp/tmp.aMFtECeDC8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits
Calibrating the magnitude scale
Found non-empty wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.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_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits and wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.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_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits and wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits.cat
Found non-empty wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits and wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits.cat
The reference image (wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits) and catalog (wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits.cat) found
'wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.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 4711 out of 7957 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.888960
a=0.000000 b=1.000000 c=22.888960
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.27
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.27
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:
2.2 pix Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
2.2 pix Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits
2.4 pix fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits
2.4 pix fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits
Limiting magnitude estimates:
15.3 mag. Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
15.3 mag. Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits
13.5 mag. fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits
13.6 mag. fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 11.0 (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.2Re6C0HO45 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits' -> 'wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
WCS_IMAGE_NAME=wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
WCS-calibrated image found: wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
Checking if the catalog wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits.cat corresponding to the image wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits alredy exist and is non-empty...
Catalog wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits.cat corresponding to the image wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
WCS catalog name: wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=512, passed=7957
Got 7957 stars (including 7436 good ones) from the SExtractor catalog wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits.cat
util/solve_plate_with_UCAC5 got 7957 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 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: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.24"
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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.23"
Estimated accuracy of the plate solution: 0.21"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits -region wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.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.6MhyLdEsOH (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits' -> 'wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits
WCS_IMAGE_NAME=wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits
WCS-calibrated image found: wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits
Checking if the catalog wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits.cat corresponding to the image wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits alredy exist and is non-empty...
Catalog wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits.cat corresponding to the image wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits
WCS catalog name: wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=499, passed=7917
Got 7917 stars (including 7409 good ones) from the SExtractor catalog wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits.cat
util/solve_plate_with_UCAC5 got 7917 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 959 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: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.24"
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 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.23"
Estimated accuracy of the plate solution: 0.20"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits -region wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.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.gJfzt1hovk (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_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.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_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits
WCS_IMAGE_NAME=wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits
WCS-calibrated image found: wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits
Checking if the catalog wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits.cat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits.cat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.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_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits
WCS catalog name: wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=139, passed=2728
Got 2728 stars (including 2587 good ones) from the SExtractor catalog wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits.cat
util/solve_plate_with_UCAC5 got 2728 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 960 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: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits -region wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.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.aMFtECeDC8 (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_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.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_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits
WCS_IMAGE_NAME=wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits
WCS-calibrated image found: wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits
Checking if the catalog wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits.cat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits.cat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.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_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits
WCS catalog name: wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=127, passed=2740
Got 2740 stars (including 2612 good ones) from the SExtractor catalog wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits.cat
util/solve_plate_with_UCAC5 got 2740 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 958 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: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits -region wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.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_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits'
Saving fully-calibrated image wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits'
Saving fully-calibrated image wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits'
Saving fully-calibrated image wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits'
Preparing the HTML report for the field Dra-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Dra-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits
SExtractor catalog cache: saved Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits.cat to cache
SExtractor catalog cache: saved Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
Creating symlink local_wcs_cache/wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits
Creating symlink local_wcs_cache/wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits
Creating symlink local_wcs_cache/wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.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_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits exists and is non-empty
wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits exists and is non-empty
wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits exists and is non-empty
wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 12:00:25.175 +69:59:06.47
Second-epoch image center 12:00:01.978 +69:59:51.64
Angular distance between the image centers 0.04 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 12:00:25.175 +69:59:06.47
Second-epoch image center 12:00:01.602 +69:59:54.16
Angular distance between the image centers 0.04 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 12:00:01.978 +69:59:51.64
Second-epoch second image center 12:00:01.602 +69:59:54.16
Angular distance between the image centers 0.00088 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00088 deg. (min. required shift: 0.00164 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/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits &> /tmp/tmp.FpJfA6QtTW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits &> /tmp/tmp.QMusl5nKB7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits &> /tmp/tmp.zoYQPrvttc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits &> /tmp/tmp.3nBHnzvLdZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits
Calibrating the magnitude scale
Found non-empty wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.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_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits and wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.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_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits and wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits.cat
Found non-empty wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits and wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits.cat
The reference image (wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits) and catalog (wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits.cat) found
'wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.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 4753 out of 40162 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.777944
a=0.000000 b=1.000000 c=22.777944
From vast_summary.log: estimated ref. image limiting mag.: -7.35
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.43
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.43
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 53 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
2.2 pix Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits
2.2 pix fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits
2.2 pix fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits
Limiting magnitude estimates:
15.4 mag. Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
15.4 mag. Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits
13.8 mag. fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits
13.8 mag. fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 13.5 (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.FpJfA6QtTW (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits' -> 'wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
WCS_IMAGE_NAME=wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
WCS-calibrated image found: wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
Checking if the catalog wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits.cat corresponding to the image wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits alredy exist and is non-empty...
Catalog wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits.cat corresponding to the image wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
WCS catalog name: wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1868, passed=40151
Got 40151 stars (including 38202 good ones) from the SExtractor catalog wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits.cat
util/solve_plate_with_UCAC5 got 40151 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 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: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.25"
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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.25"
Estimated accuracy of the plate solution: 0.21"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits -region wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.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.QMusl5nKB7 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits' -> 'wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits
WCS_IMAGE_NAME=wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits
WCS-calibrated image found: wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits
Checking if the catalog wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits.cat corresponding to the image wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits alredy exist and is non-empty...
Catalog wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits.cat corresponding to the image wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits
WCS catalog name: wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1911, passed=40557
Got 40557 stars (including 38577 good ones) from the SExtractor catalog wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits.cat
util/solve_plate_with_UCAC5 got 40557 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 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: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.25"
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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.25"
Estimated accuracy of the plate solution: 0.22"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits -region wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.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.zoYQPrvttc (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_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.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_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits
WCS_IMAGE_NAME=wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits
WCS-calibrated image found: wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits
Checking if the catalog wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits.cat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits.cat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.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_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits
WCS catalog name: wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=533, passed=17704
Got 17704 stars (including 17151 good ones) from the SExtractor catalog wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits.cat
util/solve_plate_with_UCAC5 got 17704 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 960 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: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits -region wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.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.3nBHnzvLdZ (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_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.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_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits
WCS_IMAGE_NAME=wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits
WCS-calibrated image found: wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits
Checking if the catalog wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits.cat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits.cat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.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_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits
WCS catalog name: wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=558, passed=17509
Got 17509 stars (including 16934 good ones) from the SExtractor catalog wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits.cat
util/solve_plate_with_UCAC5 got 17509 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 961 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: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits -region wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.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_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.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_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/wcs_Dra-03-Q2b1x1_2026-01-21_04-56-46_20.00sec_-14.90C_LIGHT_0526.fits
Saving fully-calibrated image wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.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_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/wcs_Dra-03-Q2b1x1_2026-01-21_04-57-28_20.00sec_-15.00C_LIGHT_0527.fits
Saving fully-calibrated image wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.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_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-08_20.00sec_-15.00C_LIGHT_0201.fits
Saving fully-calibrated image wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.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_Dra-03-Q2b1x1_062430_TTUQ2b1x1_19252_RUwDbduf/wcs_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202.fits
Preparing the HTML report for the field Dra-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52534.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52536.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52539.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52791.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52812.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53119.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53199.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53294.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53552.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53565.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out53289.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out53456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53587.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53633.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 15s
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 52534_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 52534_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
**** FOUND 12:04:04.23 +68:56:42.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)
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Considering the candidate 52536_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 52536_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
**** FOUND 13:09:49.00 +68:23:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 1.541 1685499446471399552 197.45475030049 +68.39401869789 13.3592 12.9765 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.541#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52539_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 52539_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
**** FOUND 11:50:09.76 +70:51:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 0.137 1062511072932290816 177.54058816532 +70.85441649379 11.8571 11.3793 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.137#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52791_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 52791_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
**** FOUND 12:05:58.40 +68:46:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 0.931 1682060066724778112 181.49293292852 +68.78113078403 11.8992 11.4690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.931#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52799_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 52799_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52812_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 52812_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
**** FOUND 12:14:53.92 +70:10:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 0.474 1683876391214664064 183.72436851944 +70.17036211935 12.1740 11.7138 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.474#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52815_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 52815_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53012_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53012_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53038_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53038_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53057_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53057_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53058_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53058_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53092_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53092_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53119_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53119_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
**** FOUND 12:16:56.89 +70:08:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 1.745 1683862376737459968 184.23846651243 +70.13999907447 13.1918 12.7073 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.745#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53120_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53120_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53130_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53130_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53137_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53137_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53153_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53153_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53181_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53181_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53199_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53199_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
**** FOUND 11:33:47.52 +66:52:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 1.770 1057488057140037376 173.44908599186 +66.86935569370 12.9475 12.3256 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.770#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53215_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53215_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53227_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53227_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
**** FOUND 12:15:25.99 +70:13:31.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53251_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53251_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
**** FOUND 11:03:26.61 +70:00:20.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53261_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53261_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53263_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53263_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53285_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53285_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53287_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53287_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53289_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53289_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
**** FOUND 11:59:23.38 +71:34:37.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)
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Considering the candidate 53294_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53294_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
**** FOUND 11:32:59.56 +69:31:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 1.062 1061916512019669504 173.24900812332 +69.53039737269 12.7501 12.2735 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.062#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53305_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53305_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53337_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53337_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
**** FOUND 11:20:49.60 +67:04:19.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53347_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53347_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53359_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53359_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53371_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53371_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
**** FOUND 12:41:59.24 +73:10:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 1.075 1689891789266359936 190.49774104284 +73.16763620610 13.6640 13.1121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.075#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53384_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53384_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53408_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53408_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53452_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53452_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53456_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
Preparing report for the candidate 53456_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
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Considering the candidate 53463_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53463_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53465_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53465_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
**** FOUND 11:08:15.59 +71:56:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 1.271 1075338697136761088 167.06386419850 +71.93509702644 12.9693 12.4304 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.271#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53480_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53480_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53489_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53489_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53503_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53503_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53528_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53528_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53541_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53541_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53552_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53552_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
**** FOUND 11:21:31.92 +71:44:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 0.768 1074628343905499136 170.38239076254 +71.74503999084 12.8189 12.1809 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.768#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53561_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53561_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53565_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53565_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
**** FOUND 11:44:18.34 +66:23:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 0.825 1056993173828241280 176.07595738363 +66.39235914234 13.4157 12.9117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.825#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53578_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53578_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53582_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53582_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53587_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
Preparing report for the candidate 53587_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
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Considering the candidate 53621_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53621_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53633_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
Preparing report for the candidate 53633_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
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Considering the candidate 53638_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202
The candidate 53638_fd_Dra-03-Q2b1x1_2026-03-25_06-23-50_20.00sec_-14.90C_LIGHT_0202 did not pass the final checks