This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH
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
V0890 Oph,2461128.8565,13.38,0.05,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
V0890 Oph 20260329.3565 13.38CV 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/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:26:29.98 +09:07:00.8 ;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_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20_00sec_-14_90C_LIGHT_0316_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20_00sec_-14_90C_LIGHT_0315_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20_00sec_-14_90C_LIGHT_0316_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20_00sec_-14_90C_LIGHT_0315_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
ASASSN-V J190843.37+045819.2,2461128.8565,13.04,0.05,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
ASASSN-V J190843.37+045819.2 20260329.3565 13.04CV 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/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:08:42.32 +04:58:24.9 ;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_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20_00sec_-14_90C_LIGHT_0316_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20_00sec_-14_90C_LIGHT_0315_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20_00sec_-14_90C_LIGHT_0316_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20_00sec_-14_90C_LIGHT_0315_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 29.3565* 18 53 07.94 +02 51 38.2 13.2 U Ser 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
ZTF J185308.05+025137.7,2461128.8565,13.16,0.05,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
ZTF J185308.05+025137.7 20260329.3565 13.16CV 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/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:53:07.94 +02:51:38.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20_00sec_-14_90C_LIGHT_0316_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20_00sec_-14_90C_LIGHT_0315_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20_00sec_-14_90C_LIGHT_0316_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20_00sec_-14_90C_LIGHT_0315_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: 2461121.89388564 22.03.2026 09:27:01.719 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
First image: 2461121.89388564 22.03.2026 09:27:01.719 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
Last image: 2461128.85680215 29.03.2026 08:33:37.706 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.02
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: 4 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): 13431
Objects passed selection criteria: 13401
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 10747
Average stars matched: 10534.2 (98.0204 %)
Memory usage VmPeak: 119580 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 Sun Mar 29 03:35:40 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: 2461121.89388564 22.03.2026 09:27:01.719 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
First image: 2461121.89388564 22.03.2026 09:27:01.719 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
Last image: 2461128.85680215 29.03.2026 08:33:37.706 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 103
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.70
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: 30 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): 117721
Objects passed selection criteria: 117550
Measurements per detected object (mean, median, min, max): 3.1 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 3.0 2 4
Average stars detected per image: 96478.8
Average stars matched: 92843 (96.2316 %)
Memory usage VmPeak: 1892320 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 Sun Mar 29 03:37:37 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
SExtractor catalog cache: saved Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat to cache
SExtractor catalog cache: saved Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.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/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.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: 2461128.85622448
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits exists and is non-empty
Saving wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits to local_wcs_cache/
'wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits' -> 'local_wcs_cache/wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits'
wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits exists and is non-empty
Saving wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits to local_wcs_cache/
'wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits' -> 'local_wcs_cache/wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits'
wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits exists and is non-empty
Saving wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits to local_wcs_cache/
'wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits' -> 'local_wcs_cache/wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits'
wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits exists and is non-empty
Saving wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits to local_wcs_cache/
'wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits' -> 'local_wcs_cache/wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:51:43.806 +06:00:37.02
Second-epoch image center 18:51:24.970 +06:01:29.75
Angular distance between the image centers 0.08 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:51:43.806 +06:00:37.02
Second-epoch image center 18:51:27.292 +06:01:03.64
Angular distance between the image centers 0.07 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 18:51:24.970 +06:01:29.75
Second-epoch second image center 18:51:27.292 +06:01:03.64
Angular distance between the image centers 0.01205 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/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits &> /tmp/tmp.ZXhSlVWr6q
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits &> /tmp/tmp.uC6i7lUYn6
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits &> /tmp/tmp.wSI6ciKsSh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits &> /tmp/tmp.LsK0On0xml
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
Calibrating the magnitude scale
Found non-empty wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.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_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits and wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.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_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits and wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat
Found non-empty wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits and wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat
The reference image (wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits) and catalog (wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat) found
'wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.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 10700 out of 17031 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.810355
a=0.000000 b=1.000000 c=22.810355
From vast_summary.log: estimated ref. image limiting mag.: -8.02
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.79
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.79
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:
2.1 pix Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
2.1 pix Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
2.5 pix fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits
2.5 pix fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
Limiting magnitude estimates:
14.8 mag. Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
14.8 mag. Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
14.0 mag. fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits
14.0 mag. fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.2 (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.ZXhSlVWr6q (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/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.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_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits' -> 'wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
WCS_IMAGE_NAME=wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
WCS-calibrated image found: wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
Checking if the catalog wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat corresponding to the image wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits alredy exist and is non-empty...
Catalog wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat corresponding to the image wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
WCS catalog name: wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1444, passed=17031
Got 17031 stars (including 15563 good ones) from the SExtractor catalog wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat
util/solve_plate_with_UCAC5 got 17031 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (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 945 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: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits -region wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.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.uC6i7lUYn6 (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/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.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_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits' -> 'wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
WCS_IMAGE_NAME=wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
WCS-calibrated image found: wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
Checking if the catalog wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat corresponding to the image wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits alredy exist and is non-empty...
Catalog wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat corresponding to the image wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
WCS catalog name: wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1468, passed=16916
Got 16916 stars (including 15414 good ones) from the SExtractor catalog wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat
util/solve_plate_with_UCAC5 got 16916 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
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 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits -region wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.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.wSI6ciKsSh (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_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.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_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits
WCS_IMAGE_NAME=wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits
WCS-calibrated image found: wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits
Checking if the catalog wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits.cat corresponding to the image wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits.cat corresponding to the image wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits
WCS catalog name: wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=555, passed=8227
Got 8227 stars (including 7666 good ones) from the SExtractor catalog wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits.cat
util/solve_plate_with_UCAC5 got 8227 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 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 945 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: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.71"
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 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.72"
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits -region wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.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.LsK0On0xml (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_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.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_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
WCS_IMAGE_NAME=wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
WCS-calibrated image found: wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
Checking if the catalog wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits.cat corresponding to the image wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits.cat corresponding to the image wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
WCS catalog name: wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=565, passed=8230
Got 8230 stars (including 7661 good ones) from the SExtractor catalog wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits.cat
util/solve_plate_with_UCAC5 got 8230 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 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 943 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: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.68"
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 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.68"
Estimated accuracy of the plate solution: 0.74"
Excluding outliers - 940 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits -region wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.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_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits'
Saving fully-calibrated image wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits'
Saving fully-calibrated image wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits'
Saving fully-calibrated image wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits'
Preparing the HTML report for the field Ser-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Ser-04-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/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
SExtractor catalog cache: saved Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat to cache
SExtractor catalog cache: saved Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
Creating symlink local_wcs_cache/wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
Creating symlink local_wcs_cache/wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits
Creating symlink local_wcs_cache/wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.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_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits exists and is non-empty
wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits exists and is non-empty
wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits exists and is non-empty
wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:51:43.806 +06:00:37.02
Second-epoch image center 18:51:24.970 +06:01:29.75
Angular distance between the image centers 0.08 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:51:43.806 +06:00:37.02
Second-epoch image center 18:51:27.292 +06:01:03.64
Angular distance between the image centers 0.07 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 18:51:24.970 +06:01:29.75
Second-epoch second image center 18:51:27.292 +06:01:03.64
Angular distance between the image centers 0.01205 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/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits &> /tmp/tmp.IX2QKsbbYN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits &> /tmp/tmp.f1lDkDcNUU
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits &> /tmp/tmp.2nZQzHDrnJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits &> /tmp/tmp.pbpg7h7ThZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
Calibrating the magnitude scale
Found non-empty wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.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_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits and wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.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_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits and wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat
Found non-empty wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits and wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat
The reference image (wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits) and catalog (wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat) found
'wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.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 12073 out of 147350 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.621929
a=0.000000 b=1.000000 c=22.621929
From vast_summary.log: estimated ref. image limiting mag.: -7.70
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.92
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.92
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 68 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
2.0 pix Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
2.4 pix fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits
2.4 pix fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
Limiting magnitude estimates:
14.9 mag. Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
14.9 mag. Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
14.0 mag. fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits
14.1 mag. fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
All-image limiting magnitude estimate: 14.0 (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.IX2QKsbbYN (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/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.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_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits' -> 'wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
WCS_IMAGE_NAME=wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
WCS-calibrated image found: wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
Checking if the catalog wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat corresponding to the image wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits alredy exist and is non-empty...
Catalog wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat corresponding to the image wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
WCS catalog name: wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=17153, passed=147336
Got 147336 stars (including 129905 good ones) from the SExtractor catalog wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat
util/solve_plate_with_UCAC5 got 147336 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
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 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits -region wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.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.f1lDkDcNUU (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/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.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_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits' -> 'wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
WCS_IMAGE_NAME=wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
WCS-calibrated image found: wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
Checking if the catalog wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat corresponding to the image wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits alredy exist and is non-empty...
Catalog wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat corresponding to the image wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
WCS catalog name: wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=17458, passed=150232
Got 150232 stars (including 132473 good ones) from the SExtractor catalog wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat
util/solve_plate_with_UCAC5 got 150232 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (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 945 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: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits -region wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.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.2nZQzHDrnJ (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_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.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_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits
WCS_IMAGE_NAME=wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits
WCS-calibrated image found: wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits
Checking if the catalog wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits.cat corresponding to the image wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits.cat corresponding to the image wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits
WCS catalog name: wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=4873, passed=68950
Got 68950 stars (including 63986 good ones) from the SExtractor catalog wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits.cat
util/solve_plate_with_UCAC5 got 68950 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 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 939 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: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.69"
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 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.69"
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits -region wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.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.pbpg7h7ThZ (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_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.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_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
WCS_IMAGE_NAME=wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
WCS-calibrated image found: wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
Checking if the catalog wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits.cat corresponding to the image wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits.cat corresponding to the image wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
WCS catalog name: wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=5035, passed=70520
Got 70520 stars (including 65382 good ones) from the SExtractor catalog wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits.cat
util/solve_plate_with_UCAC5 got 70520 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 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 936 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: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
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 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.66"
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits -region wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.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_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.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_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
Saving fully-calibrated image wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.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_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/wcs_Ser-04-Q2b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
Saving fully-calibrated image wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.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_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-32-47_20.00sec_-14.90C_LIGHT_0315.fits
Saving fully-calibrated image wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.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_2026-03-29_CI_Ser-04-Q2b1x1_033417_TTUQ2b1x1_26012_9KqBioPH/wcs_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316.fits
Preparing the HTML report for the field Ser-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out170701.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170716.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170717.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170722.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170728.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170731.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170736.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170752.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170755.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170757.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170761.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170927.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171144.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171154.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171172.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171173.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171174.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171175.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171184.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171233.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171254.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171256.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171286.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171326.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171329.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171335.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171343.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171394.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171401.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171447.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171516.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171576.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171609.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171623.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out171419.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18569.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42871.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
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 170701_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 170701_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:54:36.44 +06:42:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.159 4282884285985093376 283.65125942838 +06.71099251042 14.2850 13.4337 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.159#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 170716_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 170716_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:47:15.84 +08:12:53.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)
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Considering the candidate 170717_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 170717_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:42:53.14 +07:31:06.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)
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Considering the candidate 170722_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 170722_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:39:36.94 +06:32:50.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)
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Considering the candidate 170728_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 170728_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 19:05:06.09 +02:24:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 3.714 4268486146896460800 286.27493335451 +02.40409909813 12.9700 12.4780 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.714#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 170731_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 170731_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:45:05.14 +09:52:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 0.855 4503614200233408384 281.27122706384 +09.88245202750 13.6043 13.0530 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.855#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 170736_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 170736_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:49:24.76 +08:40:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 5.133 4311093940456018816 282.35387883686 +08.67392664845 13.6246 13.0098 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.133#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 170749_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 170749_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:51:04.29 +10:08:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170752_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 170752_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:34:54.17 +08:40:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 0.926 4479263865949257856 278.72593064829 +08.67813387669 13.4295 13.0767 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.926#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 170753_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 170753_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:43:12.66 +09:09:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170755_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 170755_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:34:59.85 +09:44:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 2.671 4479776165337879168 278.74912934731 +09.74852096677 13.1919 12.7117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.671#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 170757_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 170757_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:49:17.73 +10:18:19.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)
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Considering the candidate 170761_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 170761_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:38:22.51 +09:22:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 2.413 4479711676422565120 279.59410523238 +09.38248871636 13.4398 12.8473 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.413#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 170763_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 170763_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:29:20.40 +08:10:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170766_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 170766_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:56:28.80 +10:05:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170772_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 170772_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:31:59.21 +06:48:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170775_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 170775_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:54:33.37 +09:28:21.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170782_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 170782_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:30:57.61 +04:25:20.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170786_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 170786_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:35:37.85 +10:05:08.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170789_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 170789_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:36:39.74 +09:55:09.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170927_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 170927_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:37:41.53 +09:45:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 1.835 4479741912993096064 279.42253152599 +09.76188866794 10.7225 9.3494 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.835#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 170947_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 170947_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:25:31.12 +08:01:45.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 170965_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 170965_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:36:31.40 +09:05:48.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 170966_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 170966_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:36:32.40 +06:39:29.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 171039_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171039_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:30:01.14 +04:04:22.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 171082_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171082_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:56:24.67 +02:29:54.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 171144_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171144_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 19:12:40.74 +06:02:29.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)
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Considering the candidate 171154_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171154_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:47:02.65 +09:25:05.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)
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Considering the candidate 171166_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171166_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 19:12:35.60 +10:02:39.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 171172_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171172_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:32:33.13 +04:17:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 2.882 4283444762051052544 278.13725973871 +04.29145734050 11.8713 10.5699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.882#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 171173_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171173_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:32:46.88 +07:25:41.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 2.970 4478851957100589440 278.19453246535 +07.42802599440 12.2294 11.0132 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.970#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 171174_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171174_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:40:24.12 +08:50:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 0.996 4479434015382343680 280.10057859267 +08.84570663858 12.5642 11.6873 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.996#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 171175_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171175_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:33:21.65 +09:05:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.049 4479362066085312896 278.33993973053 +09.08610138699 12.9238 12.2264 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.049#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 171176_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171176_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:43:14.95 +09:59:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 171184_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171184_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:27:14.48 +05:23:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 2.116 4284555887271248640 276.81012585388 +05.38464418031 12.9543 12.3212 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.116#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 171233_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171233_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:31:01.21 +04:37:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 1.456 4284219849026974208 277.75466941194 +04.61706124580 12.9334 12.2639 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.456#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 171238_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171238_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 19:04:51.29 +03:00:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 171254_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171254_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 19:05:59.66 +07:21:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 2.875 4306776325763748224 286.49806133056 +07.35808029116 12.8050 12.1315 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.875#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 171255_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171255_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:47:29.83 +09:35:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 171256_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171256_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:26:55.50 +03:56:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 1.868 4284120102714990208 276.73134893403 +03.94431504832 12.9785 12.1907 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.868#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 171268_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171268_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:55:57.17 +07:08:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 171286_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171286_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:23:44.48 +08:27:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 2.933 4478505679653700352 275.93488442069 +08.46067809551 13.0295 12.2496 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.933#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 171320_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171320_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 19:07:23.77 +05:12:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 171325_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171325_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:33:25.44 +08:27:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 2.198 4479253489308145664 278.35649743487 +08.46294421516 13.0544 12.1428 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.198#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 171326_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171326_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:37:11.93 +02:59:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 3.364 4280060911944223360 279.29904284074 +02.99299021717 13.0723 12.2783 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.364#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 171329_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171329_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:26:25.20 +06:54:43.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)
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Considering the candidate 171335_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171335_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:35:32.73 +09:01:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 2.241 4479302275827821696 278.88579686118 +09.02083534121 12.8834 11.8547 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.241#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 171340_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171340_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:28:27.26 +03:46:15.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 171343_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171343_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:27:03.86 +06:31:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 1.354 4477224546758666880 276.76602832615 +06.52026683026 13.1119 12.5177 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.354#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 171349_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171349_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 19:01:51.35 +07:49:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 5.853 4307095325873872384 285.46295204203 +07.83106197533 13.0279 12.2677 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.853#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 171374_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171374_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:40:44.76 +08:46:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 4.462 4479429686055115904 280.18564439311 +08.77614949666 13.6900 12.9297 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 171393_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171393_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:31:21.76 +08:58:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 1.309 4479344641385936768 277.84085560157 +08.96745108674 13.2790 12.4976 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.309#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 171394_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171394_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:29:55.93 +09:09:46.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 1.042 4480021188940794624 277.48281199076 +09.16282031132 13.3203 12.7903 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.042#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 171401_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171401_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:40:18.48 +09:42:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 1.198 4479635015537139072 280.07691551731 +09.70940544806 12.7114 11.6807 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.198#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 171419_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
Preparing report for the candidate 171419_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
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Considering the candidate 171424_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171424_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:53:53.27 +06:01:26.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 171447_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171447_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:41:32.19 +09:02:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 5.708 4479443803589760384 280.38437268872 +09.04617762232 12.2960 10.9445 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.708#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 171516_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171516_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:43:02.65 +07:42:49.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 3.040 4286952818312826752 280.76123574786 +07.71451659384 13.4524 12.8174 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.040#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 171528_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171528_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:33:57.12 +05:41:27.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 171531_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171531_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:49:07.92 +08:59:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 0.855 4311161697862886784 282.28323608949 +08.99146187269 13.4397 12.7039 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.855#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 171576_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171576_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:33:15.42 +05:25:50.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 0.920 4284698445827064704 278.31411714989 +05.43053118631 13.3852 12.6826 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.920#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 171609_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171609_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:54:51.26 +09:13:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 3.037 4310472063540876288 283.71281621064 +09.23018343442 13.6044 12.7328 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.037#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 171623_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 171623_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:39:49.94 +05:12:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 1.391 4283937235871118464 279.95818154916 +05.19995946623 13.1944 12.1100 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.391#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 158436_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 158436_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 19:14:09.88 +05:04:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53108_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 53108_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks
**** FOUND 18:40:04.13 +05:41:13.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 42871_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
Preparing report for the candidate 42871_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
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Considering the candidate 18569_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
Preparing report for the candidate 18569_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
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Considering the candidate 48452_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316
The candidate 48452_fd_Ser-04-Q2b1x1_2026-03-29_03-33-37_20.00sec_-14.90C_LIGHT_0316 did not pass the final checks