This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1821684029027212544,2461135.9653,12.02,0.05,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
Gaia DR3 1821684029027212544 20260405.4653 12.02CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J310.4293+22.9588,2461135.9653,12.03,0.05,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
ATO J310.4293+22.9588 20260405.4653 12.03CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1821695058504053376,2461135.9653,11.83,0.05,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
Gaia DR3 1821695058504053376 20260405.4653 11.83CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1843208717140275072,2461135.9653,12.43,0.05,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
Gaia DR3 1843208717140275072 20260405.4653 12.43CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J297.6291+17.7507,2461135.9653,11.84,0.05,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
ATO J297.6291+17.7507 20260405.4653 11.84CV 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: 2461098.99517851 27.02.2026 11:52:53.423 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
First image: 2461098.99517851 27.02.2026 11:52:53.423 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Last image: 2461135.96566733 05.04.2026 11:10:23.657 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.96
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 20299
Objects passed selection criteria: 20168
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 12361.5
Average stars matched: 12005 (97.116 %)
Memory usage VmPeak: 125568 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 5 06:41:06 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: 2461098.99517851 27.02.2026 11:52:53.423 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
First image: 2461098.99517851 27.02.2026 11:52:53.423 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Last image: 2461135.96566733 05.04.2026 11:10:23.657 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 72
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.61
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: 41 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): 193476
Objects passed selection criteria: 192837
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 124894
Average stars matched: 119788 (95.9123 %)
Memory usage VmPeak: 2022416 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 5 06:47:30 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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
SExtractor catalog cache: saved Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat to cache
SExtractor catalog cache: saved Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.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: 2461135.96500714
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_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits exists and is non-empty
Saving wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits to local_wcs_cache/
'wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits' -> 'local_wcs_cache/wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits'
wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits exists and is non-empty
Saving wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits to local_wcs_cache/
'wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits' -> 'local_wcs_cache/wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits'
wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits exists and is non-empty
Saving wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits to local_wcs_cache/
'wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits' -> 'local_wcs_cache/wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits'
wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits exists and is non-empty
Saving wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits to local_wcs_cache/
'wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits' -> 'local_wcs_cache/wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 20:18:28.950 +22:00:14.29
Second-epoch image center 20:18:47.009 +22:00:18.63
Angular distance between the image centers 0.0698 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 20:18:28.950 +22:00:14.29
Second-epoch image center 20:18:45.792 +21:59:44.61
Angular distance between the image centers 0.0656 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 20:18:47.009 +22:00:18.63
Second-epoch second image center 20:18:45.792 +21:59:44.61
Angular distance between the image centers 0.01056 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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits &> /tmp/tmp.PLAc040voq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits &> /tmp/tmp.MGOZsP3x8B
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits &> /tmp/tmp.MDeR4iD2yv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits &> /tmp/tmp.8PLrqwgTiH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
Calibrating the magnitude scale
Found non-empty wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
Found non-empty wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
The reference image (wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits) and catalog (wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat) found
'wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat' -> 'wcsmag.cat'
Read 24638 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 295.6627 to 313.2570 deg, Dec +16.3767 to +27.3369 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 295.6627 to 313.2570 deg, Dec 16.3767 to 27.3369 deg
Loaded 24193 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): 13464 out of 14549 total matches.
Matched with Tycho-2 14549 out of 24638 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.758582
a=0.000000 b=1.000000 c=22.758582
From vast_summary.log: estimated ref. image limiting mag.: -7.96
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.80
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.80
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
2.0 pix Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
2.6 pix fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits
2.7 pix fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
Limiting magnitude estimates:
14.8 mag. Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
14.8 mag. Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
11.8 mag. fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits
11.9 mag. fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
All-image limiting magnitude estimate: 11.8 (SNR ) 9.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.PLAc040voq (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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits' -> 'wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS_IMAGE_NAME=wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS-calibrated image found: wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Checking if the catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits alredy exist and is non-empty...
Catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS catalog name: wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2463, passed=24638
Got 24638 stars (including 22152 good ones) from the SExtractor catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
util/solve_plate_with_UCAC5 got 24638 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 23512 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 23512 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
WARNING: Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 23512 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 935 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits -region wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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.MGOZsP3x8B (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/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits' -> 'wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS-calibrated image found: wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Checking if the catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS catalog name: wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2477, passed=24779
Got 24779 stars (including 22281 good ones) from the SExtractor catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat
util/solve_plate_with_UCAC5 got 24779 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 23741 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
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 531 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 23740 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 23740 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits -region wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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.MDeR4iD2yv (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_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.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_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits
WCS_IMAGE_NAME=wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits
WCS-calibrated image found: wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits
Checking if the catalog wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits
WCS catalog name: wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=245, passed=3763
Got 3763 stars (including 3515 good ones) from the SExtractor catalog wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits.cat
util/solve_plate_with_UCAC5 got 3763 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 3692 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 3693 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
WARNING: Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 3693 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 924 stars left (next iteration limit 1016)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits -region wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.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.8PLrqwgTiH (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_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.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_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
WCS_IMAGE_NAME=wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
WCS-calibrated image found: wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
Checking if the catalog wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
WCS catalog name: wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=237, passed=3694
Got 3694 stars (including 3455 good ones) from the SExtractor catalog wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits.cat
util/solve_plate_with_UCAC5 got 3694 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 3588 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 3588 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
WARNING: Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 3588 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits -region wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.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_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits'
Saving fully-calibrated image wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits'
Saving fully-calibrated image wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits'
Saving fully-calibrated image wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits'
Preparing the HTML report for the field Vul-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Vul-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
SExtractor catalog cache: saved Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat to cache
SExtractor catalog cache: saved Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Creating symlink local_wcs_cache/wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Creating symlink local_wcs_cache/wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits
Creating symlink local_wcs_cache/wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.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_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits exists and is non-empty
wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits exists and is non-empty
wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits exists and is non-empty
wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 20:18:28.950 +22:00:14.29
Second-epoch image center 20:18:47.009 +22:00:18.63
Angular distance between the image centers 0.0698 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 20:18:28.950 +22:00:14.29
Second-epoch image center 20:18:45.792 +21:59:44.61
Angular distance between the image centers 0.0656 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 20:18:47.009 +22:00:18.63
Second-epoch second image center 20:18:45.792 +21:59:44.61
Angular distance between the image centers 0.01056 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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits &> /tmp/tmp.zr7IXS4WRE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits &> /tmp/tmp.GHCKgCYzHk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits &> /tmp/tmp.tvJMjbGWIq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits &> /tmp/tmp.tAdFpaxiMW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
Calibrating the magnitude scale
Found non-empty wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
Found non-empty wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
The reference image (wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits) and catalog (wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat) found
'wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat' -> 'wcsmag.cat'
Read 232861 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 295.6471 to 313.2612 deg, Dec +16.3395 to +27.3423 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 295.6471 to 313.2612 deg, Dec 16.3395 to 27.3423 deg
Loaded 24297 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): 12337 out of 17496 total matches.
Matched with Tycho-2 17496 out of 232861 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.547121
a=0.000000 b=1.000000 c=22.547121
From vast_summary.log: estimated ref. image limiting mag.: -7.61
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.94
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.94
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 30 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.8 pix Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
1.9 pix Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
2.2 pix fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits
2.2 pix fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
Limiting magnitude estimates:
14.9 mag. Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
14.9 mag. Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
12.8 mag. fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits
12.7 mag. fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
All-image limiting magnitude estimate: 12.7 (SNR ) 12.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.zr7IXS4WRE (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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits' -> 'wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS_IMAGE_NAME=wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS-calibrated image found: wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Checking if the catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits alredy exist and is non-empty...
Catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS catalog name: wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=34, blended=33174, passed=232827
Got 232827 stars (including 199306 good ones) from the SExtractor catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
util/solve_plate_with_UCAC5 got 232827 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 228418 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 228419 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
WARNING: Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 228415 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 941 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits -region wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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.GHCKgCYzHk (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/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits' -> 'wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS-calibrated image found: wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Checking if the catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS catalog name: wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=51, blended=32901, passed=232172
Got 232172 stars (including 198927 good ones) from the SExtractor catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat
util/solve_plate_with_UCAC5 got 232172 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 227885 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
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 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 227886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
WARNING: Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 227886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits -region wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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.tvJMjbGWIq (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_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.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_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits
WCS_IMAGE_NAME=wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits
WCS-calibrated image found: wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits
Checking if the catalog wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits
WCS catalog name: wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1988, passed=44326
Got 44326 stars (including 42281 good ones) from the SExtractor catalog wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits.cat
util/solve_plate_with_UCAC5 got 44326 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 43679 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 922 matched stars entering correct_measured_positions(), 43681 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
WARNING: Accuracy estimation diagnostic: 922 matched stars entering correct_measured_positions(), 43681 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 922 stars left (next iteration limit 1015)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits -region wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.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.tAdFpaxiMW (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_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.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_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
WCS_IMAGE_NAME=wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
WCS-calibrated image found: wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
Checking if the catalog wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
WCS catalog name: wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=2065, passed=42568
Got 42568 stars (including 40451 good ones) from the SExtractor catalog wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits.cat
util/solve_plate_with_UCAC5 got 42568 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 41571 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
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 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 41572 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
WARNING: Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 41572 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 929 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits -region wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.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_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Saving fully-calibrated image wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Saving fully-calibrated image wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.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_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-09-26_20.00sec_-5.00C_LIGHT_0297.fits
Saving fully-calibrated image wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.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_2026-04-05_CI_Vul-02-Q2b1x1_063604_TTUQ2b1x1_23311_G5yEKzUd/wcs_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298.fits
Preparing the HTML report for the field Vul-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out246041.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262755.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262777.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out174892.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262727.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28924.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62016.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 262707_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
The candidate 262707_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298 did not pass the final checks
**** FOUND 20:32:44.94 +19:22:01.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262724_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
The candidate 262724_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298 did not pass the final checks
**** FOUND 20:34:46.85 +25:53:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262727_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
Preparing report for the candidate 262727_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262730_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
The candidate 262730_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298 did not pass the final checks
**** FOUND 20:39:14.81 +21:57:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262735_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
The candidate 262735_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298 did not pass the final checks
**** FOUND 20:35:56.66 +25:46:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262736_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
The candidate 262736_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298 did not pass the final checks
**** FOUND 20:36:30.56 +24:01:44.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262745_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
The candidate 262745_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298 did not pass the final checks
**** FOUND 20:43:54.96 +23:51:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262755_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
The candidate 262755_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298 did not pass the final checks
**** FOUND 20:43:47.24 +21:53:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 0.392 1817994205394923008 310.94694500171 +21.89332767245 12.7039 12.1597 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.392#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 262756_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
The candidate 262756_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298 did not pass the final checks
**** FOUND 20:36:24.81 +21:40:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262761_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
Preparing report for the candidate 262761_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
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Considering the candidate 262768_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
The candidate 262768_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298 did not pass the final checks
**** FOUND 20:21:41.76 +19:39:46.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)
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Considering the candidate 262769_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
The candidate 262769_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298 did not pass the final checks
**** FOUND 20:33:56.81 +22:27:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262771_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
The candidate 262771_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298 did not pass the final checks
**** FOUND 20:36:14.69 +22:58:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262772_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
The candidate 262772_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298 did not pass the final checks
**** FOUND 20:40:09.09 +25:16:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262777_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
The candidate 262777_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298 did not pass the final checks
**** FOUND 19:52:02.06 +21:20:11.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)
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Considering the candidate 262778_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
The candidate 262778_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298 did not pass the final checks
**** FOUND 20:40:39.08 +25:45:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262785_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
The candidate 262785_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298 did not pass the final checks
**** FOUND 20:41:55.17 +21:36:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262787_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
The candidate 262787_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298 did not pass the final checks
**** FOUND 20:44:12.38 +24:06:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262881_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
The candidate 262881_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298 did not pass the final checks
**** FOUND 20:38:30.17 +21:10:11.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 262914_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
The candidate 262914_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298 did not pass the final checks
**** FOUND 20:42:41.49 +25:28:33.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262921_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
The candidate 262921_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298 did not pass the final checks
**** FOUND 20:36:33.61 +20:44:18.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62016_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
Preparing report for the candidate 62016_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
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Considering the candidate 174892_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
Preparing report for the candidate 174892_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
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Considering the candidate 246041_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
The candidate 246041_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298 did not pass the final checks
**** FOUND 20:45:05.52 +24:10:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 1.662 1843256820773168000 311.27350460114 +24.17513116574 12.8514 12.0048 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254705_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
The candidate 254705_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298 did not pass the final checks
Rejecting candidate due to large distance (36.8") between the two second-epoch detections
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Considering the candidate 28924_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
Preparing report for the candidate 28924_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
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Considering the candidate 60371_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
The candidate 60371_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298 did not pass the final checks
**** FOUND 19:52:33.42 +19:06:26.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74911_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
The candidate 74911_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298 did not pass the final checks
**** FOUND 19:58:46.15 +19:29:35.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 182870_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
The candidate 182870_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298 did not pass the final checks
**** FOUND 19:53:28.34 +24:04:46.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 231923_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298
The candidate 231923_fd_Vul-02-Q2b1x1_2026-04-05_06-10-23_20.00sec_-4.90C_LIGHT_0298 did not pass the final checks