This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0885 Oph,2461150.9693,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
V0885 Oph 20260420.4693 12.47CV 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
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 04 20.4693* 18 23 13.61 +04 34 48.8 11.8 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J182313.51+043448.6,2461150.9693,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J182313.51+043448.6 20260420.4693 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461121.89388564 22.03.2026 09:27:01.719 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
First image: 2461121.89388564 22.03.2026 09:27:01.719 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
Last image: 2461150.96972597 20.04.2026 11:16:14.324 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.04
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 16252
Objects passed selection criteria: 16203
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 11343.5
Average stars matched: 10987 (96.8572 %)
Memory usage VmPeak: 120868 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 20 07:07:13 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461121.89388564 22.03.2026 09:27:01.719 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
First image: 2461121.89388564 22.03.2026 09:27:01.719 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
Last image: 2461150.96972597 20.04.2026 11:16:14.324 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 37
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.75
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: 57 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): 136507
Objects passed selection criteria: 136219
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 99041.2
Average stars matched: 94081 (94.9917 %)
Memory usage VmPeak: 1898636 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 20 07:11:28 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/TTUQ1b1x1/TTUQ1_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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
SExtractor catalog cache: saved Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat to cache
SExtractor catalog cache: saved Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.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: 2461150.96886911
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'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits exists and is non-empty
Saving wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits to local_wcs_cache/
'wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits' -> 'local_wcs_cache/wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits'
wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits exists and is non-empty
Saving wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits to local_wcs_cache/
'wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits' -> 'local_wcs_cache/wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits'
wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits exists and is non-empty
Saving wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits to local_wcs_cache/
'wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits' -> 'local_wcs_cache/wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits'
wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits exists and is non-empty
Saving wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits to local_wcs_cache/
'wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits' -> 'local_wcs_cache/wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits (1st reference image)
verification OK: wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
Image size: 942.3'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:51:43.806 +06:00:37.02 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits (1st new image)
verification OK: wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:51:36.149 +06:00:07.73 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:51:43.806 +06:00:37.02
Second-epoch image center 18:51:36.149 +06:00:07.73
Angular distance between the image centers 0.0328 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits (2nd new image)
verification OK: wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:51:38.806 +06:00:30.10 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:51:43.806 +06:00:37.02
Second-epoch image center 18:51:38.806 +06:00:30.10
Angular distance between the image centers 0.0208 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 18:51:36.149 +06:00:07.73
Second-epoch second image center 18:51:38.806 +06:00:30.10
Angular distance between the image centers 0.01264 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits &> /tmp/tmp.xP9tM2zhYb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits &> /tmp/tmp.5WAvXMl7Id
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits &> /tmp/tmp.AqlHwf4HkI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits &> /tmp/tmp.mKsvqyN4Hu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
Calibrating the magnitude scale
Found non-empty wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits and wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits and wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat
Found non-empty wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits and wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat
The reference image (wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits) and catalog (wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat) found
'wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat' -> 'wcsmag.cat'
Read 17031 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.8858 to 290.8648 deg, Dec +0.6585 to +11.3165 deg
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
Tycho-2 catalog search boundaries: RA 274.8858 to 290.8648 deg, Dec 0.6585 to 11.3165 deg
Loaded 13648 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 10048 out of 10700 total matches.
Matched with Tycho-2 10700 out of 17031 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.817454
a=0.000000 b=1.000000 c=22.817454
From vast_summary.log: estimated ref. image limiting mag.: -8.04
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.78
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.78
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: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
2.1 pix Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
3.1 pix fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits
3.0 pix fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
Limiting magnitude estimates:
14.8 mag. Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
14.8 mag. Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
14.2 mag. fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits
13.8 mag. fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 11.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.xP9tM2zhYb (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits' -> 'wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
WCS_IMAGE_NAME=wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
WCS-calibrated image found: wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
Checking if the catalog wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat corresponding to the image wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits alredy exist and is non-empty...
Catalog wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat corresponding to the image wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
WCS catalog name: wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1444, passed=17031
Got 17031 stars (including 15563 good ones) from the SExtractor catalog wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat
util/solve_plate_with_UCAC5 got 17031 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 16279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 16279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 16279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits -region wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.5WAvXMl7Id (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits' -> 'wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
WCS_IMAGE_NAME=wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
WCS-calibrated image found: wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
Checking if the catalog wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat corresponding to the image wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits alredy exist and is non-empty...
Catalog wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat corresponding to the image wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
WCS catalog name: wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1468, passed=16916
Got 16916 stars (including 15414 good ones) from the SExtractor catalog wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat
util/solve_plate_with_UCAC5 got 16916 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 16028 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 16028 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 16028 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits -region wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.AqlHwf4HkI (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_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.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_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits
WCS_IMAGE_NAME=wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits
WCS-calibrated image found: wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits
Checking if the catalog wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits.cat corresponding to the image wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits.cat corresponding to the image wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits
WCS catalog name: wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=429, passed=6374
Got 6374 stars (including 5938 good ones) from the SExtractor catalog wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits.cat
util/solve_plate_with_UCAC5 got 6374 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 892 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 6024 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
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...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 6022 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 6022 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 940 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits -region wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.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.mKsvqyN4Hu (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_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.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_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
WCS_IMAGE_NAME=wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
WCS-calibrated image found: wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
Checking if the catalog wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits.cat corresponding to the image wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits.cat corresponding to the image wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
WCS catalog name: wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=332, passed=5321
Got 5321 stars (including 4984 good ones) from the SExtractor catalog wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits.cat
util/solve_plate_with_UCAC5 got 5321 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 5149 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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...
Searching UCAC5 zones 451 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 5148 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 5149 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 941 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits -region wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits'
Saving fully-calibrated image wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits'
Saving fully-calibrated image wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits'
Saving fully-calibrated image wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits'
Preparing the HTML report for the field Ser-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20918.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20918_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053
The candidate 20918_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053 did not pass the final checks
**** FOUND 18:22:24.12 +08:54:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 0.288 4478723314231260032 275.60057266433 +08.90025753646 11.8060 11.2849 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.288#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21183_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053
The candidate 21183_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053 did not pass the final checks
**** FOUND 18:23:36.48 +09:32:38.0 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Ser-04-Q1b1x1 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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
SExtractor catalog cache: saved Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat to cache
SExtractor catalog cache: saved Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
Creating symlink local_wcs_cache/wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
Creating symlink local_wcs_cache/wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits
Creating symlink local_wcs_cache/wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits exists and is non-empty
wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits exists and is non-empty
wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits exists and is non-empty
wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits (1st reference image)
verification OK: wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
Image size: 942.3'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:51:43.806 +06:00:37.02 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits (1st new image)
verification OK: wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:51:36.149 +06:00:07.73 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:51:43.806 +06:00:37.02
Second-epoch image center 18:51:36.149 +06:00:07.73
Angular distance between the image centers 0.0328 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits (2nd new image)
verification OK: wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:51:38.806 +06:00:30.10 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:51:43.806 +06:00:37.02
Second-epoch image center 18:51:38.806 +06:00:30.10
Angular distance between the image centers 0.0208 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 18:51:36.149 +06:00:07.73
Second-epoch second image center 18:51:38.806 +06:00:30.10
Angular distance between the image centers 0.01264 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits &> /tmp/tmp.skf8Am48y1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits &> /tmp/tmp.9ZIxlIiQz5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits &> /tmp/tmp.80cHJhKUGp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits &> /tmp/tmp.OuAaFr0hUc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
Calibrating the magnitude scale
Found non-empty wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits and wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits and wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat
Found non-empty wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits and wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat
The reference image (wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits) and catalog (wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat) found
'wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat' -> 'wcsmag.cat'
Read 147350 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.8613 to 290.8654 deg, Dec +0.6327 to +11.3181 deg
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
Tycho-2 catalog search boundaries: RA 274.8613 to 290.8654 deg, Dec 0.6327 to 11.3181 deg
Loaded 13685 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 9356 out of 12073 total matches.
Matched with Tycho-2 12073 out of 147350 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.635822
a=0.000000 b=1.000000 c=22.635822
From vast_summary.log: estimated ref. image limiting mag.: -7.75
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.89
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.89
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 22 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
2.0 pix Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
2.9 pix fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits
2.8 pix fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
Limiting magnitude estimates:
14.9 mag. Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
14.9 mag. Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
14.3 mag. fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits
13.8 mag. fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 13.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.skf8Am48y1 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits' -> 'wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
WCS_IMAGE_NAME=wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
WCS-calibrated image found: wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
Checking if the catalog wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat corresponding to the image wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits alredy exist and is non-empty...
Catalog wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat corresponding to the image wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
WCS catalog name: wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=17153, passed=147332
Got 147332 stars (including 129901 good ones) from the SExtractor catalog wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat
util/solve_plate_with_UCAC5 got 147332 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 143550 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 143549 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 143550 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits -region wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.9ZIxlIiQz5 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits' -> 'wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
WCS_IMAGE_NAME=wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
WCS-calibrated image found: wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
Checking if the catalog wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat corresponding to the image wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits alredy exist and is non-empty...
Catalog wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat corresponding to the image wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
WCS catalog name: wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=17458, passed=150227
Got 150227 stars (including 132468 good ones) from the SExtractor catalog wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat
util/solve_plate_with_UCAC5 got 150227 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 146131 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 146130 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 146130 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits -region wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.80cHJhKUGp (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_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.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_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits
WCS_IMAGE_NAME=wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits
WCS-calibrated image found: wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits
Checking if the catalog wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits.cat corresponding to the image wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits.cat corresponding to the image wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits
WCS catalog name: wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=3769, passed=56287
Got 56287 stars (including 52451 good ones) from the SExtractor catalog wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits.cat
util/solve_plate_with_UCAC5 got 56287 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 893 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 53235 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 53236 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 53236 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits -region wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.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.OuAaFr0hUc (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_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.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_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
WCS_IMAGE_NAME=wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
WCS-calibrated image found: wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
Checking if the catalog wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits.cat corresponding to the image wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits.cat corresponding to the image wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
WCS catalog name: wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=2431, passed=45002
Got 45002 stars (including 42480 good ones) from the SExtractor catalog wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits.cat
util/solve_plate_with_UCAC5 got 45002 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 42989 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 42990 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 42989 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits -region wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/wcs_Ser-04-Q1b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits
Saving fully-calibrated image wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/wcs_Ser-04-Q1b1x1_2026-03-22_04-28-08_20.00sec_-14.90C_LIGHT_0268.fits
Saving fully-calibrated image wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.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_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-15-00_20.00sec_-5.00C_LIGHTs_0052.fits
Saving fully-calibrated image wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.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_2026-04-20_CI_Ser-04-Q1b1x1_061713_TTUQ1b1x1_568078_tlxJq7W1/wcs_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053.fits
Preparing the HTML report for the field Ser-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out158140.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out172919.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174324.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174658.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174929.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175355.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out135874.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39978.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 172919_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053
The candidate 172919_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053 did not pass the final checks
**** FOUND 18:24:45.94 +08:37:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 2.133 4478531728643315840 276.19196863445 +08.62615781807 13.2842 12.7426 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.133#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 172924_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053
The candidate 172924_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053 did not pass the final checks
**** FOUND 19:21:47.84 +06:38:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173210_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053
The candidate 173210_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053 did not pass the final checks
**** FOUND 18:25:31.07 +08:01:44.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 173721_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053
The candidate 173721_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053 did not pass the final checks
**** FOUND 19:07:23.78 +05:12:05.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173739_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053
The candidate 173739_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053 did not pass the final checks
**** FOUND 19:02:06.94 +01:26:23.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173915_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053
The candidate 173915_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053 did not pass the final checks
**** FOUND 18:23:58.96 +09:53:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174121_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053
The candidate 174121_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053 did not pass the final checks
**** FOUND 18:26:08.95 +09:58:28.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174324_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053
The candidate 174324_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053 did not pass the final checks
**** FOUND 18:23:06.48 +05:22:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 1.876 4476635994486280960 275.77748298533 +05.38199356507 13.7182 12.8442 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.876#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174551_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053
The candidate 174551_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053 did not pass the final checks
**** FOUND 18:25:23.77 +04:47:57.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174658_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053
The candidate 174658_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053 did not pass the final checks
**** FOUND 19:19:53.74 +06:19:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 2.432 4294054392118197760 289.97457753172 +06.32821320587 12.2443 10.9166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.432#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174929_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053
The candidate 174929_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053 did not pass the final checks
**** FOUND 18:27:08.63 +08:00:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 1.590 4477687819111722624 276.78638655214 +08.01345683509 13.7087 13.1968 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.590#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174962_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053
The candidate 174962_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053 did not pass the final checks
**** FOUND 18:26:00.90 +08:35:03.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 175116_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053
The candidate 175116_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053 did not pass the final checks
**** FOUND 18:29:02.98 +10:34:51.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 175355_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053
The candidate 175355_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053 did not pass the final checks
**** FOUND 18:22:43.40 +08:29:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 3.501 4478691570140637440 275.68168009145 +08.48921646489 14.0435 13.1909 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.501#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51198_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053
The candidate 51198_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053 did not pass the final checks
**** FOUND 18:30:49.74 +05:30:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 135874_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053
Preparing report for the candidate 135874_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053
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Considering the candidate 158140_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053
The candidate 158140_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053 did not pass the final checks
**** FOUND 18:25:48.57 +06:11:06.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)
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Considering the candidate 35265_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053
The candidate 35265_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053 did not pass the final checks
**** FOUND 18:21:44.27 +04:09:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116113_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053
The candidate 116113_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053 did not pass the final checks
**** FOUND 18:24:24.33 +09:59:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78474_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053
The candidate 78474_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053 did not pass the final checks
**** FOUND 19:22:46.49 +07:26:55.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39978_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053
Preparing report for the candidate 39978_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053
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Considering the candidate 50461_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053
The candidate 50461_fd_Ser-04-Q1b1x1_2026-04-20_06-16-14_20.00sec_-4.90C_LIGHTs_0053 did not pass the final checks