This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP
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!
TCP 2026 03 26.3028* 15 18 29.72 +02 07 18.1 13.4 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
target,2461125.8028,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.3028 13.44CV 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-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:18:29.72 +02:07:18.1 ;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-05-Q2b1x1_2026-02-22_05-29-54_20_00sec_-14_90C_LIGHT_0565_fits__*pix.png resample_wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20_00sec_-10_00C_LIGHT_0561_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20_00sec_-14_90C_LIGHT_0565_fits__*pix.png resample_wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20_00sec_-10_00C_LIGHT_0560_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20_00sec_-14_90C_LIGHT_0565_fits__*pix.png resample_wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20_00sec_-10_00C_LIGHT_0561_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20_00sec_-14_90C_LIGHT_0565_fits__*pix.png resample_wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20_00sec_-10_00C_LIGHT_0560_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 26.3028* 15 49 42.10 +02 06 59.0 13.8 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
VARIABLE_NAME,2461125.8028,13.82,0.05,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
VARIABLE_NAME 20260326.3028 13.82CV 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-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:49:42.10 +02:06:59.0 ;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-05-Q2b1x1_2026-02-22_05-29-54_20_00sec_-14_90C_LIGHT_0565_fits__*pix.png resample_wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20_00sec_-10_00C_LIGHT_0561_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20_00sec_-14_90C_LIGHT_0565_fits__*pix.png resample_wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20_00sec_-10_00C_LIGHT_0560_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20_00sec_-14_90C_LIGHT_0565_fits__*pix.png resample_wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20_00sec_-10_00C_LIGHT_0561_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20_00sec_-14_90C_LIGHT_0565_fits__*pix.png resample_wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20_00sec_-10_00C_LIGHT_0560_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 26.3028* 15 26 55.60 +00 02 56.4 14.8 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
VARIABLE_NAME,2461125.8028,14.76,0.05,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
VARIABLE_NAME 20260326.3028 14.76CV 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-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:26:55.60 +00:02:56.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20_00sec_-14_90C_LIGHT_0565_fits__*pix.png resample_wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20_00sec_-10_00C_LIGHT_0561_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20_00sec_-14_90C_LIGHT_0565_fits__*pix.png resample_wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20_00sec_-10_00C_LIGHT_0560_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20_00sec_-14_90C_LIGHT_0565_fits__*pix.png resample_wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20_00sec_-10_00C_LIGHT_0561_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20_00sec_-14_90C_LIGHT_0565_fits__*pix.png resample_wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20_00sec_-10_00C_LIGHT_0560_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: 2461093.97922028 22.02.2026 11:29:54.632 /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
First image: 2461093.97922028 22.02.2026 11:29:54.632 /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
Last image: 2461125.80301727 26.03.2026 07:16:10.692 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.66
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6493
Objects passed selection criteria: 6487
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 5794.75
Average stars matched: 5694.75 (98.2743 %)
Memory usage VmPeak: 113232 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 Thu Mar 26 02:21:05 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: 2461093.97922028 22.02.2026 11:29:54.632 /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
First image: 2461093.97922028 22.02.2026 11:29:54.632 /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
Last image: 2461125.80301727 26.03.2026 07:16:10.692 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 58
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.38
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: 15 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): 42712
Objects passed selection criteria: 42631
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 38842.8
Average stars matched: 37782.2 (97.2698 %)
Memory usage VmPeak: 146492 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 Thu Mar 26 02:21:50 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-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
SExtractor catalog cache: saved Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits.cat to cache
SExtractor catalog cache: saved Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.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-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.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: 2461125.80252177
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits exists and is non-empty
Saving wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits to local_wcs_cache/
'wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits' -> 'local_wcs_cache/wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits'
wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits exists and is non-empty
Saving wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits to local_wcs_cache/
'wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits' -> 'local_wcs_cache/wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits'
wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits exists and is non-empty
Saving wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits to local_wcs_cache/
'wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits' -> 'local_wcs_cache/wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits'
wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits exists and is non-empty
Saving wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits to local_wcs_cache/
'wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits' -> 'local_wcs_cache/wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.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 15:25:48.421 -02:00:22.04
Second-epoch image center 15:26:00.611 -02:00:34.10
Angular distance between the image centers 0.05 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 15:25:48.421 -02:00:22.04
Second-epoch image center 15:26:00.428 -02:00:36.17
Angular distance between the image centers 0.05 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 15:26:00.611 -02:00:34.10
Second-epoch second image center 15:26:00.428 -02:00:36.17
Angular distance between the image centers 0.00096 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00096 deg. (min. required shift: 0.00164 deg.)
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits &> /tmp/tmp.SoucDLA1JH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits &> /tmp/tmp.mBT2YqtWPy
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits &> /tmp/tmp.13U1QcbJ31
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits &> /tmp/tmp.ANTUcljzGN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
Calibrating the magnitude scale
Found non-empty wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.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-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits and wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.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-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits and wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits.cat
Found non-empty wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits and wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits.cat
The reference image (wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits) and catalog (wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits.cat) found
'wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.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 3935 out of 8222 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.934262
a=0.000000 b=1.000000 c=22.934262
From vast_summary.log: estimated ref. image limiting mag.: -7.66
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.27
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.27
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
2.2 pix Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits
2.4 pix fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits
2.4 pix fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
Limiting magnitude estimates:
15.3 mag. Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
15.3 mag. Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits
14.7 mag. fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits
14.7 mag. fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 11.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.SoucDLA1JH (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-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.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_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.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-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.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-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits' -> 'wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
WCS_IMAGE_NAME=wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
WCS-calibrated image found: wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
Checking if the catalog wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits.cat corresponding to the image wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits alredy exist and is non-empty...
Catalog wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits.cat corresponding to the image wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
WCS catalog name: wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=559, passed=8222
Got 8222 stars (including 7648 good ones) from the SExtractor catalog wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits.cat
util/solve_plate_with_UCAC5 got 8222 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits -region wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.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.mBT2YqtWPy (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-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.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_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.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-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.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-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits' -> 'wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits
WCS_IMAGE_NAME=wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits
WCS-calibrated image found: wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits
Checking if the catalog wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits.cat corresponding to the image wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits alredy exist and is non-empty...
Catalog wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits.cat corresponding to the image wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits
WCS catalog name: wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=570, passed=8221
Got 8221 stars (including 7645 good ones) from the SExtractor catalog wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits.cat
util/solve_plate_with_UCAC5 got 8221 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits -region wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.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.13U1QcbJ31 (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_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.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_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits
WCS_IMAGE_NAME=wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits
WCS-calibrated image found: wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits
Checking if the catalog wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits.cat corresponding to the image wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits.cat corresponding to the image wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits
WCS catalog name: wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=376, passed=5758
Got 5758 stars (including 5373 good ones) from the SExtractor catalog wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits.cat
util/solve_plate_with_UCAC5 got 5758 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits -region wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.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.ANTUcljzGN (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_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.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_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
WCS_IMAGE_NAME=wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
WCS-calibrated image found: wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
Checking if the catalog wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits.cat corresponding to the image wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits.cat corresponding to the image wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
WCS catalog name: wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=390, passed=5731
Got 5731 stars (including 5334 good ones) from the SExtractor catalog wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits.cat
util/solve_plate_with_UCAC5 got 5731 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits -region wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.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-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits'
Saving fully-calibrated image wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits'
Saving fully-calibrated image wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits'
Saving fully-calibrated image wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits'
Preparing the HTML report for the field Ser-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02739_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 02739_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:45:48.62 -03:50:30.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01085_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 01085_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:11:41.33 -06:00:40.9 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Ser-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
SExtractor catalog cache: saved Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits.cat to cache
SExtractor catalog cache: saved Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.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-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
Creating symlink local_wcs_cache/wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits
Creating symlink local_wcs_cache/wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits
Creating symlink local_wcs_cache/wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.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-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits exists and is non-empty
wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits exists and is non-empty
wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits exists and is non-empty
wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.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 15:25:48.421 -02:00:22.04
Second-epoch image center 15:26:00.611 -02:00:34.10
Angular distance between the image centers 0.05 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 15:25:48.421 -02:00:22.04
Second-epoch image center 15:26:00.428 -02:00:36.17
Angular distance between the image centers 0.05 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 15:26:00.611 -02:00:34.10
Second-epoch second image center 15:26:00.428 -02:00:36.17
Angular distance between the image centers 0.00096 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00096 deg. (min. required shift: 0.00164 deg.)
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits &> /tmp/tmp.A019RzR58d
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits &> /tmp/tmp.VTph6Ol6IO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits &> /tmp/tmp.SECqaONU1P
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits &> /tmp/tmp.hbHZucjzYT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
Calibrating the magnitude scale
Found non-empty wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.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-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits and wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.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-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits and wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits.cat
Found non-empty wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits and wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits.cat
The reference image (wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits) and catalog (wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits.cat) found
'wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.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 3963 out of 51984 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.824449
a=0.000000 b=1.000000 c=22.824449
From vast_summary.log: estimated ref. image limiting mag.: -7.38
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.44
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.44
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 42 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
2.0 pix Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits
2.2 pix fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits
2.2 pix fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
Limiting magnitude estimates:
15.4 mag. Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
15.5 mag. Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits
14.9 mag. fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits
15.0 mag. fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 14.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.A019RzR58d (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-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.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_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.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-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.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-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits' -> 'wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
WCS_IMAGE_NAME=wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
WCS-calibrated image found: wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
Checking if the catalog wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits.cat corresponding to the image wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits alredy exist and is non-empty...
Catalog wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits.cat corresponding to the image wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
WCS catalog name: wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=2145, passed=51967
Got 51967 stars (including 49706 good ones) from the SExtractor catalog wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits.cat
util/solve_plate_with_UCAC5 got 51967 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits -region wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.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.VTph6Ol6IO (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-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.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_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.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-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.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-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits' -> 'wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits
WCS_IMAGE_NAME=wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits
WCS-calibrated image found: wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits
Checking if the catalog wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits.cat corresponding to the image wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits alredy exist and is non-empty...
Catalog wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits.cat corresponding to the image wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits
WCS catalog name: wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=2199, passed=52225
Got 52225 stars (including 49928 good ones) from the SExtractor catalog wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits.cat
util/solve_plate_with_UCAC5 got 52225 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 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: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
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 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits -region wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.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.SECqaONU1P (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_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.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_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits
WCS_IMAGE_NAME=wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits
WCS-calibrated image found: wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits
Checking if the catalog wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits.cat corresponding to the image wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits.cat corresponding to the image wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits
WCS catalog name: wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1516, passed=36632
Got 36632 stars (including 35072 good ones) from the SExtractor catalog wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits.cat
util/solve_plate_with_UCAC5 got 36632 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits -region wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.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.hbHZucjzYT (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_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.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_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
WCS_IMAGE_NAME=wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
WCS-calibrated image found: wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
Checking if the catalog wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits.cat corresponding to the image wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits.cat corresponding to the image wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
WCS catalog name: wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=1521, passed=37040
Got 37040 stars (including 35479 good ones) from the SExtractor catalog wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits.cat
util/solve_plate_with_UCAC5 got 37040 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits -region wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.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-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.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_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits
Saving fully-calibrated image wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.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_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/wcs_Ser-05-Q2b1x1_2026-02-22_05-30-42_20.00sec_-15.00C_LIGHT_0566.fits
Saving fully-calibrated image wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.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_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits
Saving fully-calibrated image wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.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_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits
Preparing the HTML report for the field Ser-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out65719.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65727.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65728.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65731.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65732.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65733.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65734.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65740.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65742.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65745.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65792.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65803.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65826.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65838.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65861.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65873.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65875.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65883.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65906.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65907.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65908.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65916.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65954.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65993.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out65749.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65867.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65979.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 65719_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65719_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:32:39.53 -02:29:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.76, MAG_FAINT_SEARCH_LIMIT=15.74)GAIADR2_OUTPUT=# 1.525 4414270840260048000 233.16436150596 -02.48753411881 14.8431 14.1470 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.525#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65727_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65727_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:40:45.83 -00:47:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 0.756 4416379325605732992 235.19074975614 -00.78797654149 14.8650 14.1807 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.756#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65728_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65728_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:08:52.58 -02:26:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 0.777 6339577479305404288 227.21908123727 -02.43625628687 14.2997 13.6307 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.777#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65731_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65731_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:41:13.97 +01:27:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.65, MAG_FAINT_SEARCH_LIMIT=15.63)GAIADR2_OUTPUT=# 3.833 4422944097218129152 235.30789601405 +01.46351794131 14.1278 13.0916 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.833#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65732_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65732_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:21:11.89 -01:20:08.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)
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Considering the candidate 65733_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65733_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:29:44.68 -01:36:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.57, MAG_FAINT_SEARCH_LIMIT=15.55)GAIADR2_OUTPUT=# 1.480 4414578566076803968 232.43575556253 -01.60811767973 14.8388 14.1978 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.480#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65734_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65734_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:40:35.50 +01:48:52.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 1.310 4423716779014755712 235.14790257939 +01.81480796974 14.5593 13.9912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.310#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65740_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65740_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:08:17.24 -01:13:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 2.296 4418347691936918144 227.07193751283 -01.22620418921 14.1213 13.4515 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.296#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65742_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65742_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:50:01.52 +01:12:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 1.545 4422723335900433280 237.50627598941 +01.20982472812 13.8666 13.1687 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.545#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65745_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65745_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:08:14.59 +01:18:47.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)
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Considering the candidate 65749_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
Preparing report for the candidate 65749_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
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Considering the candidate 65751_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65751_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:48:03.87 -02:28:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 1.743 4403146737529227648 237.01582441185 -02.47098142727 13.3488 12.8015 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.743#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65783_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65783_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 65786_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65786_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 65792_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65792_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:18:45.26 +02:04:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 3.365 4421572280371888640 229.68920908005 +02.07505597971 12.3118 11.5180 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.365#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65794_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65794_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 65797_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65797_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 65798_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65798_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:45:46.29 +00:53:52.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 65803_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65803_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:41:59.76 +00:28:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 0.562 4416620530968989824 235.49905895820 +00.47972783282 12.6968 12.1468 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.562#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65816_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65816_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 65822_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65822_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:18:41.09 +02:02:52.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65826_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65826_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:39:19.83 -00:25:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 0.523 4416454603496284032 234.83267806636 -00.43135734182 13.3950 12.7800 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.523#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65831_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65831_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 65838_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65838_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:08:31.82 -00:59:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 2.562 4418425684247023232 227.13221917668 -00.98502734173 13.2970 12.6320 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.562#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65849_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65849_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 65857_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65857_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:49:42.37 -03:27:31.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 65861_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65861_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:50:12.06 +00:12:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 1.660 4410590431248940160 237.54998842213 +00.21268526791 13.6181 13.0339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.660#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65867_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
Preparing report for the candidate 65867_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
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Considering the candidate 65873_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65873_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:38:03.13 -04:54:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 2.627 4400903184048534400 234.51246859464 -04.90262898342 14.0917 13.5232 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.627#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65875_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65875_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:35:46.94 +01:08:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 1.426 4417690115264466688 233.94597085955 +01.14586025506 13.8655 13.2975 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.426#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65883_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65883_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:25:43.85 -01:13:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 2.736 4415414607230792960 231.43263346873 -01.23038258749 13.9238 13.2398 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.736#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65906_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65906_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:31:40.42 +00:50:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 0.491 4417760243489975424 232.91833673116 +00.84519513637 14.5892 14.1317 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.491#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65907_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65907_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:46:13.44 +00:39:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 5.809 4422597613616470656 236.55755961655 +00.65716908597 14.0504 13.5460 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.809#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65908_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65908_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:34:09.27 -04:44:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 4.626 4400955479570276736 233.53755920073 -04.73624901048 14.1819 13.5475 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.626#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65916_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65916_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:48:58.51 -00:08:46.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 0.141 4410471855790115328 237.24381830172 -00.14636198023 14.2972 13.7523 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.141#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65954_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65954_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:50:16.68 -00:20:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 0.730 4410275696045983744 237.56968288115 -00.33421781490 14.1789 13.6504 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65979_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
Preparing report for the candidate 65979_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
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Considering the candidate 65984_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65984_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 65993_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65993_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:46:56.38 -01:19:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 0.686 4404171757243075072 236.73498249682 -01.32709894590 14.6650 14.1116 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.686#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65994_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 65994_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 06234_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 06234_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks
**** FOUND 15:11:41.34 -06:00:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17214_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561
The candidate 17214_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561 did not pass the final checks