This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my
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
NSVS J0411418+790654,2461147.8425,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0411418+790654 20260417.3425 11.27CV 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 17.3425* 03 12 48.31 +73 56 29.9 13.6 U Cas 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
ZTF J031248.11+735627.7,2461147.8425,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J031248.11+735627.7 20260417.3425 13.61CV 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!
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 J042321.54+741240.7,2461147.8425,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J042321.54+741240.7 20260417.3425 12.54CV 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: 2461049.69447938 09.01.2026 04:39:53.018 /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
First image: 2461049.69447938 09.01.2026 04:39:53.018 /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
Last image: 2461147.84278808 17.04.2026 08:13:26.890 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
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): 12705
Objects passed selection criteria: 12667
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 10394.5
Average stars matched: 9993.25 (96.1398 %)
Memory usage VmPeak: 118280 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 Fri Apr 17 03:28:51 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: 2461049.69447938 09.01.2026 04:39:53.018 /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
First image: 2461049.69447938 09.01.2026 04:39:53.018 /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
Last image: 2461147.84278808 17.04.2026 08:13:26.890 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 69
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.21
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: 31 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): 87469
Objects passed selection criteria: 87255
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 71797.8
Average stars matched: 68529.5 (95.448 %)
Memory usage VmPeak: 1874876 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 Fri Apr 17 03:30:33 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
SExtractor catalog cache: saved Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits.cat to cache
SExtractor catalog cache: saved Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.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/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.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: 2461147.84219690
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_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits exists and is non-empty
Saving wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits to local_wcs_cache/
'wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits' -> 'local_wcs_cache/wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits'
wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits exists and is non-empty
Saving wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits to local_wcs_cache/
'wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits' -> 'local_wcs_cache/wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits'
wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits exists and is non-empty
Saving wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits to local_wcs_cache/
'wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits' -> 'local_wcs_cache/wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits'
wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits exists and is non-empty
Saving wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits to local_wcs_cache/
'wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits' -> 'local_wcs_cache/wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits (1st reference image)
verification OK: wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
Image size: 941.5'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: 04:00:01.055 +77:29:57.29 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_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits (1st new image)
verification OK: wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits
Image size: 937.1'x624.8' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 03:59:58.922 +77:29:59.68 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:00:01.055 +77:29:57.29
Second-epoch image center 03:59:58.922 +77:29:59.68
Angular distance between the image centers 0.0020 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits (2nd new image)
verification OK: wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
Image size: 937.1'x624.8' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 03:59:58.260 +77:30:25.97 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:00:01.055 +77:29:57.29
Second-epoch image center 03:59:58.260 +77:30:25.97
Angular distance between the image centers 0.0084 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 03:59:58.922 +77:29:59.68
Second-epoch second image center 03:59:58.260 +77:30:25.97
Angular distance between the image centers 0.00733 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/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits &> /tmp/tmp.TAnVsi1Mue
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits &> /tmp/tmp.YQq1JjQt1W
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits &> /tmp/tmp.0Z92l6toQ4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits &> /tmp/tmp.U2gwJbvENe
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.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_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits and wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.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_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits and wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits.cat
Found non-empty wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits and wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits.cat
The reference image (wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits) and catalog (wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits.cat) found
'wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits.cat' -> 'wcsmag.cat'
Read 16361 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 10.9999 to 103.4512 deg, Dec +69.5819 to +83.1399 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 10.9999 to 103.4512 deg, Dec 69.5819 to 83.1399 deg
Loaded 18140 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): 8370 out of 9000 total matches.
Matched with Tycho-2 9000 out of 16361 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.903663
a=0.000000 b=1.000000 c=22.903663
From vast_summary.log: estimated ref. image limiting mag.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.36
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.36
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
2.0 pix Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits
2.4 pix fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits
2.4 pix fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
Limiting magnitude estimates:
15.4 mag. Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
15.4 mag. Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits
14.6 mag. fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits
14.6 mag. fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 11.8 (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.TAnVsi1Mue (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits' -> 'wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
WCS_IMAGE_NAME=wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
WCS-calibrated image found: wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
Checking if the catalog wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits.cat corresponding to the image wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits alredy exist and is non-empty...
Catalog wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits.cat corresponding to the image wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
WCS catalog name: wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1344, passed=16361
Got 16361 stars (including 14997 good ones) from the SExtractor catalog wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits.cat
util/solve_plate_with_UCAC5 got 16361 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 797 to 867 (Dec 69.6 to 83.1)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 16092 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 797 to 867 (Dec 69.6 to 83.1)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 16093 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 16093 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits -region wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.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.YQq1JjQt1W (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits' -> 'wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits
WCS_IMAGE_NAME=wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits
WCS-calibrated image found: wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits
Checking if the catalog wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits.cat corresponding to the image wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits alredy exist and is non-empty...
Catalog wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits.cat corresponding to the image wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits
WCS catalog name: wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1323, passed=16218
Got 16218 stars (including 14876 good ones) from the SExtractor catalog wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits.cat
util/solve_plate_with_UCAC5 got 16218 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 797 to 867 (Dec 69.6 to 83.2)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 15983 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
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 797 to 867 (Dec 69.6 to 83.2)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 15983 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 15983 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits -region wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.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.0Z92l6toQ4 (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_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.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_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits
WCS_IMAGE_NAME=wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits
WCS-calibrated image found: wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits
Checking if the catalog wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits.cat corresponding to the image wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits.cat corresponding to the image wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits
WCS catalog name: wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=650, passed=10004
Got 10004 stars (including 9345 good ones) from the SExtractor catalog wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits.cat
util/solve_plate_with_UCAC5 got 10004 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 803 to 865 (Dec 70.7 to 82.8)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 9853 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
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 803 to 865 (Dec 70.7 to 82.8)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 9852 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 9854 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 966 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits -region wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.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.U2gwJbvENe (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_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.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_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
WCS_IMAGE_NAME=wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
WCS-calibrated image found: wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
Checking if the catalog wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits.cat corresponding to the image wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits.cat corresponding to the image wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
WCS catalog name: wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=694, passed=9968
Got 9968 stars (including 9265 good ones) from the SExtractor catalog wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits.cat
util/solve_plate_with_UCAC5 got 9968 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 803 to 865 (Dec 70.7 to 82.8)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 9771 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
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 803 to 865 (Dec 70.7 to 82.8)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 9772 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 9774 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 965 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits -region wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.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_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits'
Saving fully-calibrated image wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits'
Saving fully-calibrated image wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits'
Saving fully-calibrated image wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits'
Preparing the HTML report for the field Cam-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out21489.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out05365.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21163_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 21163_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 03:16:53.43 +80:09:47.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21254_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 21254_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 05:22:04.39 +79:14:45.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21489_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 21489_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 05:38:53.67 +79:57:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 0.673 553805937985967488 084.72461328827 +79.96301716345 12.1380 11.6978 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.673#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05365_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
Preparing report for the candidate 05365_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04552_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 04552_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 04:39:53.37 +79:07:50.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Cam-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
04:11:42.35 +79:06:53.1
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
SExtractor catalog cache: saved Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits.cat to cache
SExtractor catalog cache: saved Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
Creating symlink local_wcs_cache/wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.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_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits exists and is non-empty
wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits exists and is non-empty
wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits exists and is non-empty
wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits (1st reference image)
verification OK: wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
Image size: 941.5'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: 04:00:01.055 +77:29:57.29 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_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits (1st new image)
verification OK: wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits
Image size: 937.1'x624.8' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 03:59:58.922 +77:29:59.68 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:00:01.055 +77:29:57.29
Second-epoch image center 03:59:58.922 +77:29:59.68
Angular distance between the image centers 0.0020 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits (2nd new image)
verification OK: wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
Image size: 937.1'x624.8' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 03:59:58.260 +77:30:25.97 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:00:01.055 +77:29:57.29
Second-epoch image center 03:59:58.260 +77:30:25.97
Angular distance between the image centers 0.0084 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 03:59:58.922 +77:29:59.68
Second-epoch second image center 03:59:58.260 +77:30:25.97
Angular distance between the image centers 0.00733 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/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits &> /tmp/tmp.f7TqfVVEgU
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits &> /tmp/tmp.43ihVa7ONA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits &> /tmp/tmp.8A92bG2zy8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits &> /tmp/tmp.m2eljyfB6q
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.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_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits and wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.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_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits and wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits.cat
Found non-empty wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits and wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits.cat
The reference image (wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits) and catalog (wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits.cat) found
'wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits.cat' -> 'wcsmag.cat'
Read 111259 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 10.9605 to 103.8707 deg, Dec +69.5589 to +83.1453 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 10.9605 to 103.8707 deg, Dec 69.5589 to 83.1453 deg
Loaded 18250 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): 7278 out of 9109 total matches.
Matched with Tycho-2 9109 out of 111259 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.771929
a=0.000000 b=1.000000 c=22.771929
From vast_summary.log: estimated ref. image limiting mag.: -7.21
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.56
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.56
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 57 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.9 pix Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
1.9 pix Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits
2.3 pix fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits
2.3 pix fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
Limiting magnitude estimates:
15.6 mag. Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
15.6 mag. Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits
14.7 mag. fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits
14.7 mag. fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.2 (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.f7TqfVVEgU (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits' -> 'wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
WCS_IMAGE_NAME=wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
WCS-calibrated image found: wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
Checking if the catalog wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits.cat corresponding to the image wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits alredy exist and is non-empty...
Catalog wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits.cat corresponding to the image wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
WCS catalog name: wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=30, blended=9167, passed=111229
Got 111229 stars (including 101869 good ones) from the SExtractor catalog wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits.cat
util/solve_plate_with_UCAC5 got 111229 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 797 to 867 (Dec 69.6 to 83.1)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 109984 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 797 to 867 (Dec 69.6 to 83.1)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 109982 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 109982 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits -region wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.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.43ihVa7ONA (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits' -> 'wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits
WCS_IMAGE_NAME=wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits
WCS-calibrated image found: wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits
Checking if the catalog wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits.cat corresponding to the image wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits alredy exist and is non-empty...
Catalog wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits.cat corresponding to the image wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits
WCS catalog name: wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=25, blended=9221, passed=111540
Got 111540 stars (including 102140 good ones) from the SExtractor catalog wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits.cat
util/solve_plate_with_UCAC5 got 111540 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 797 to 867 (Dec 69.6 to 83.2)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 110298 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 797 to 867 (Dec 69.6 to 83.2)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 110299 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 110299 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits -region wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.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.8A92bG2zy8 (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_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.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_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits
WCS_IMAGE_NAME=wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits
WCS-calibrated image found: wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits
Checking if the catalog wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits.cat corresponding to the image wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits.cat corresponding to the image wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits
WCS catalog name: wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=4365, passed=61309
Got 61309 stars (including 56874 good ones) from the SExtractor catalog wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits.cat
util/solve_plate_with_UCAC5 got 61309 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 803 to 865 (Dec 70.6 to 82.8)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 60119 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
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 803 to 865 (Dec 70.6 to 82.8)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 60118 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 60117 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits -region wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.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.m2eljyfB6q (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_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.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_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
WCS_IMAGE_NAME=wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
WCS-calibrated image found: wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
Checking if the catalog wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits.cat corresponding to the image wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits.cat corresponding to the image wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
WCS catalog name: wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=4377, passed=61146
Got 61146 stars (including 56695 good ones) from the SExtractor catalog wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits.cat
util/solve_plate_with_UCAC5 got 61146 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 803 to 865 (Dec 70.6 to 82.8)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 60005 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
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 803 to 865 (Dec 70.6 to 82.8)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 60004 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 60004 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits -region wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.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_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.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_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/wcs_Cam-03-Q2b1x1_2026-01-08_22-39-53_20.00sec_-14.90C_LIGHT_0167.fits
Saving fully-calibrated image wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.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_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/wcs_Cam-03-Q2b1x1_2026-01-08_22-40-40_20.00sec_-15.00C_LIGHT_0168.fits
Saving fully-calibrated image wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.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_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-12-35_20.00sec_-4.90C_LIGHT_0293.fits
Saving fully-calibrated image wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.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_2026-04-17_CI_Cam-03-Q2b1x1_031519_TTUQ2b1x1_3525266_L4Lt19my/wcs_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294.fits
Preparing the HTML report for the field Cam-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out129376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129382.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131029.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131889.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132104.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132507.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132700.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132765.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132890.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133307.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out100292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out88814.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129371_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 129371_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 03:18:27.82 +76:00:02.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129374_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 129374_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 03:11:54.46 +77:16:34.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129376_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 129376_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 05:21:07.46 +73:47:48.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129382_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 129382_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 03:42:37.47 +73:39:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 2.310 544530835851427200 055.65546082238 +73.65716952428 13.8059 13.2717 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.310#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129385_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 129385_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 04:03:46.70 +74:43:31.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129388_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 129388_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 04:00:54.67 +76:09:22.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129393_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 129393_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 05:17:15.96 +73:34:58.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129394_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 129394_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 05:06:48.86 +78:01:32.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129397_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 129397_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 03:45:06.48 +78:02:18.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129400_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 129400_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 05:53:28.46 +78:06:10.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129402_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 129402_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 04:20:28.14 +74:29:15.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129846_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 129846_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 03:16:53.41 +80:09:47.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129912_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 129912_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 03:50:36.17 +80:18:06.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130573_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 130573_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 03:39:48.64 +75:45:07.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130726_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 130726_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 05:14:14.59 +76:27:25.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130871_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 130871_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 03:06:47.84 +79:26:48.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130922_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 130922_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 04:27:23.74 +80:51:12.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130927_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 130927_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 03:06:13.13 +75:30:09.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130985_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 130985_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 05:00:07.74 +79:43:52.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131029_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 131029_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 05:48:16.61 +80:02:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 2.809 553645237489741184 087.06642240195 +80.04713611566 13.7596 13.1052 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.809#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131169_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 131169_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 05:15:15.85 +75:44:36.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131224_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 131224_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 04:49:09.53 +75:57:36.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131240_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 131240_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 03:48:29.46 +80:19:07.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131349_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 131349_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 04:15:13.80 +76:18:24.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131582_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 131582_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 04:45:25.66 +80:31:55.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131733_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 131733_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 04:32:09.66 +75:18:11.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131752_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 131752_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 04:19:15.83 +74:37:15.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131771_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 131771_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 05:29:50.04 +77:58:37.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131889_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 131889_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 04:50:30.50 +75:56:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 1.404 551770364006038016 072.62860801755 +75.94848847782 13.5963 13.0881 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.404#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131919_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 131919_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 05:41:15.78 +75:42:18.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131943_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 131943_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 02:58:30.17 +77:04:21.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132014_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 132014_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 03:54:15.57 +74:39:40.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132104_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 132104_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 04:51:28.19 +75:13:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 1.962 503636184484277376 072.86936649721 +75.22053238883 13.6944 13.0860 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.962#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132142_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 132142_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 04:43:59.95 +79:46:54.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132159_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 132159_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 05:42:20.81 +79:18:43.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132276_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 132276_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 06:09:04.53 +78:02:43.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132373_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 132373_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 04:50:16.43 +72:56:16.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132443_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 132443_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 04:26:20.60 +79:39:14.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132447_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 132447_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 03:50:50.11 +78:20:50.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132496_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 132496_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 03:55:31.46 +76:00:23.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132498_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 132498_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 03:57:09.33 +77:25:11.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132507_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 132507_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 05:27:52.74 +77:40:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 2.189 552340666943721472 081.97254322127 +77.66713187013 13.7724 13.0594 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.189#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132519_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 132519_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 02:54:25.09 +79:03:34.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132560_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 132560_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 04:50:46.17 +73:38:14.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132585_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 132585_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 04:34:05.08 +76:24:13.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132631_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 132631_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 05:18:11.35 +75:56:08.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132700_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 132700_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 04:54:26.20 +79:05:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 0.693 553337064995590400 073.60816430018 +79.09507771194 11.9482 10.2836 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.693#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132765_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 132765_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 04:35:24.53 +80:17:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 1.300 556611548062175360 068.85007054474 +80.28903720580 14.2188 13.5318 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.300#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132890_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 132890_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 05:14:10.85 +80:26:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 1.831 556838631572955904 078.54249756642 +80.44632069720 14.2677 13.6898 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.831#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133041_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 133041_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 04:24:19.67 +75:27:20.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133307_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 133307_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 03:36:28.06 +78:31:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 3.974 555324844579684736 054.11879710108 +78.52623926893 14.3390 13.5942 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.974#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133567_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 133567_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 03:50:20.73 +75:31:24.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33685_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 33685_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
**** FOUND 04:11:42.30 +79:06:53.4 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 88814_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
Preparing report for the candidate 88814_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
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Considering the candidate 97553_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 97553_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 100292_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
Preparing report for the candidate 100292_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
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Considering the candidate 28278_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294
The candidate 28278_fd_Cam-03-Q2b1x1_2026-04-17_03-13-26_20.00sec_-4.90C_LIGHT_0294 did not pass the final checks