This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.1977* 09 42 41.01 +08 07 50.9 13.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3854816367446718464,2461136.6977,13.21,0.05,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 3854816367446718464 20260406.1977 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.1977* 09 32 06.08 +08 47 19.1 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.6977,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.1977 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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
VARIABLE_NAME,2461136.6977,14.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.1977 14.01CV 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
VARIABLE_NAME,2461136.6977,14.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.1977 14.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.1977* 09 39 14.26 +09 53 22.2 14.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.6977,14.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.1977 14.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.74633115 22.02.2026 05:54:33.011 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
First image: 2461093.74633115 22.02.2026 05:54:33.011 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Last image: 2461136.69799315 06.04.2026 04:44:56.608 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.65
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): 9214
Objects passed selection criteria: 9187
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 7584.25
Average stars matched: 7124.75 (93.9414 %)
Memory usage VmPeak: 114052 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 23:59:44 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.74633115 22.02.2026 05:54:33.011 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
First image: 2461093.74633115 22.02.2026 05:54:33.011 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Last image: 2461136.69799315 06.04.2026 04:44:56.608 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 106
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.36
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: 20 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): 52070
Objects passed selection criteria: 51910
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 44743.2
Average stars matched: 41687.5 (93.1705 %)
Memory usage VmPeak: 148088 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 Mon Apr 6 00:00:43 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/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
SExtractor catalog cache: saved Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat to cache
SExtractor catalog cache: saved Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.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/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.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: 2461136.69730958
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_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits exists and is non-empty
Saving wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits to local_wcs_cache/
'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits' -> 'local_wcs_cache/wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits'
wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits exists and is non-empty
Saving wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits to local_wcs_cache/
'wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits' -> 'local_wcs_cache/wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits'
wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits exists and is non-empty
Saving wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits to local_wcs_cache/
'wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits' -> 'local_wcs_cache/wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits'
wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits exists and is non-empty
Saving wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits to local_wcs_cache/
'wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits' -> 'local_wcs_cache/wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits'
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:25:43.014 +06:00:02.92
Second-epoch image center 09:25:48.150 +05:59:23.43
Angular distance between the image centers 0.0239 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 09:25:43.014 +06:00:02.92
Second-epoch image center 09:25:45.259 +06:00:05.62
Angular distance between the image centers 0.0093 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 09:25:48.150 +05:59:23.43
Second-epoch second image center 09:25:45.259 +06:00:05.62
Angular distance between the image centers 0.01676 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/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits &> /tmp/tmp.pSn30GvpaI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits &> /tmp/tmp.VnCAes5kkI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits &> /tmp/tmp.IvqUYIhEtd
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits &> /tmp/tmp.oobbF2DGMq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.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_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.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_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
Found non-empty wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
The reference image (wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits) and catalog (wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat) found
'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat' -> 'wcsmag.cat'
Read 9705 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 133.2099 to 149.7640 deg, Dec +0.1004 to +11.7220 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 133.2099 to 149.7640 deg, Dec 0.1004 to 11.7220 deg
Loaded 6611 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): 4811 out of 5047 total matches.
Matched with Tycho-2 5047 out of 9705 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.925124
a=0.000000 b=1.000000 c=22.925124
From vast_summary.log: estimated ref. image limiting mag.: -7.65
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.28
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.28
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
2.5 pix Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
2.5 pix fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
2.5 pix fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
Limiting magnitude estimates:
15.3 mag. Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
15.3 mag. Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
15.1 mag. fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
15.1 mag. fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 12.1 (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.pSn30GvpaI (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits' -> 'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS-calibrated image found: wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Checking if the catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS catalog name: wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=629, passed=9705
Got 9705 stars (including 9071 good ones) from the SExtractor catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
util/solve_plate_with_UCAC5 got 9705 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 450 to 510 (Dec 0.1 to 11.7)
Done reading UCAC5 zone files...
Matched 942 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: 939 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 9526 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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 450 to 510 (Dec 0.1 to 11.7)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 9526 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
WARNING: Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 9526 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 939 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits -region wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.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.VnCAes5kkI (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits' -> 'wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS-calibrated image found: wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Checking if the catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS catalog name: wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=616, passed=9704
Got 9704 stars (including 9075 good ones) from the SExtractor catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat
util/solve_plate_with_UCAC5 got 9704 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 450 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 940 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(), 926 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 9534 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 450 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 9536 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
WARNING: Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 9537 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 937 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_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits -region wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.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.IvqUYIhEtd (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_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.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_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
Checking if the catalog wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.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_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
WCS catalog name: wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=526, passed=8746
Got 8746 stars (including 8207 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.cat
util/solve_plate_with_UCAC5 got 8746 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 942 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: 939 matched stars entering correct_measured_positions(), 929 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 8511 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 8508 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
WARNING: Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 8508 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 939 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits -region wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.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.oobbF2DGMq (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_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.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_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
Checking if the catalog wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.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_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
WCS catalog name: wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=540, passed=8716
Got 8716 stars (including 8165 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.cat
util/solve_plate_with_UCAC5 got 8716 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 8513 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 8513 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 8513 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits -region wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.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_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits'
Saving fully-calibrated image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits'
Saving fully-calibrated image wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits'
Saving fully-calibrated image wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits'
Preparing the HTML report for the field Hya-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out21273.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21358.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21425.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21273_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 21273_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:36:49.00 +09:27:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 1.442 588594103634115712 144.20443624021 +09.45346639769 12.3249 11.8021 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.442#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21358_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 21358_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:10:19.57 +04:55:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 0.930 580043824475632000 137.58179307537 +04.92540927439 12.2293 11.7856 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.930#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21425_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 21425_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:17:57.05 +07:05:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 1.502 586811455983536128 139.48809043826 +07.08743703672 12.2671 11.7108 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.502#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Hya-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/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
SExtractor catalog cache: saved Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat to cache
SExtractor catalog cache: saved Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Creating symlink local_wcs_cache/wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.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_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits exists and is non-empty
wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits exists and is non-empty
wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits exists and is non-empty
wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits exists and is non-empty
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:25:43.014 +06:00:02.92
Second-epoch image center 09:25:48.150 +05:59:23.43
Angular distance between the image centers 0.0239 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 09:25:43.014 +06:00:02.92
Second-epoch image center 09:25:45.259 +06:00:05.62
Angular distance between the image centers 0.0093 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 09:25:48.150 +05:59:23.43
Second-epoch second image center 09:25:45.259 +06:00:05.62
Angular distance between the image centers 0.01676 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/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits &> /tmp/tmp.nAkmi3XkEd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits &> /tmp/tmp.ErkUR5irVg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits &> /tmp/tmp.Vl3m7SyXYe
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits &> /tmp/tmp.AXhrhBxe5G
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.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_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.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_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
Found non-empty wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
The reference image (wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits) and catalog (wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat) found
'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat' -> 'wcsmag.cat'
Read 52265 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 133.1873 to 149.7640 deg, Dec +0.0999 to +11.7791 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 133.1873 to 149.7640 deg, Dec 0.0999 to 11.7791 deg
Loaded 6657 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): 4491 out of 5088 total matches.
Matched with Tycho-2 5088 out of 52265 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.799339
a=0.000000 b=1.000000 c=22.799339
From vast_summary.log: estimated ref. image limiting mag.: -7.36
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.44
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.44
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 54 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
2.3 pix Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
2.2 pix fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
2.2 pix fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
Limiting magnitude estimates:
15.4 mag. Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
15.4 mag. Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
15.3 mag. fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
15.3 mag. fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 14.7 (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.nAkmi3XkEd (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits' -> 'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS-calibrated image found: wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Checking if the catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS catalog name: wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=3222, passed=52238
Got 52238 stars (including 48939 good ones) from the SExtractor catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
util/solve_plate_with_UCAC5 got 52238 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 450 to 510 (Dec 0.1 to 11.8)
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: 935 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 51515 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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 450 to 510 (Dec 0.1 to 11.8)
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: 935 matched stars entering correct_measured_positions(), 51515 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
WARNING: Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 51515 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits -region wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.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.ErkUR5irVg (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits' -> 'wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS-calibrated image found: wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Checking if the catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS catalog name: wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=3213, passed=52136
Got 52136 stars (including 48850 good ones) from the SExtractor catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat
util/solve_plate_with_UCAC5 got 52136 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 450 to 510 (Dec 0.1 to 11.8)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 51370 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 450 to 510 (Dec 0.1 to 11.8)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 51371 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 51371 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 934 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_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits -region wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.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.Vl3m7SyXYe (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_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.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_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
Checking if the catalog wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.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_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
WCS catalog name: wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=28, blended=2568, passed=49541
Got 49541 stars (including 46911 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.cat
util/solve_plate_with_UCAC5 got 49541 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 48335 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 936 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(), 48338 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
WARNING: Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 48338 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits -region wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.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.AXhrhBxe5G (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_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.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_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
Checking if the catalog wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.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_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
WCS catalog name: wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=2598, passed=49994
Got 49994 stars (including 47340 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.cat
util/solve_plate_with_UCAC5 got 49994 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 938 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: 937 matched stars entering correct_measured_positions(), 928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 48845 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 48844 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
WARNING: Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 48844 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 937 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits -region wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.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_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.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_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Saving fully-calibrated image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.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_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Saving fully-calibrated image wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.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_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
Saving fully-calibrated image wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.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_Hya-02-Q2b1x1_234617_TTUQ2b1x1_11867_GYjJ9zCs/wcs_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
Preparing the HTML report for the field Hya-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out65592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65597.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65598.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65599.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65613.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65614.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65615.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65620.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65629.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out69322.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out69360.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out69436.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out69672.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out69962.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70153.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70264.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70441.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70459.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70516.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70604.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70753.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70755.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70818.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70842.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70926.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70931.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70972.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70998.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71105.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71145.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71248.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71336.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out65625.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67100.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69280.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69948.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71271.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 65592_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 65592_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:16:11.52 +08:07:49.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.83, MAG_FAINT_SEARCH_LIMIT=15.81)GAIADR2_OUTPUT=# 2.148 587146222914539264 139.04855810641 +08.13013555094 14.8196 14.2814 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.148#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65594_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 65594_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:13:15.35 +06:31:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.74, MAG_FAINT_SEARCH_LIMIT=15.72)GAIADR2_OUTPUT=# 2.103 580869145391325312 138.31449732369 +06.52140564546 14.6467 14.1425 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.103#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65597_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 65597_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:04:51.80 +02:55:44.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 2.839 577526801842034944 136.21645582875 +02.92857046344 15.2048 14.6705 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.839#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65598_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 65598_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:11:20.60 +08:56:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 2.165 590428570066121216 137.83638378532 +08.94970150877 14.6370 14.0963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.165#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65599_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 65599_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:12:52.40 +02:48:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.59, MAG_FAINT_SEARCH_LIMIT=15.57)GAIADR2_OUTPUT=# 1.060 578750283405837312 138.21838576535 +02.80409909181 14.5716 14.0219 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.060#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65611_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 65611_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:47:45.08 +04:08:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65612_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 65612_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:25:55.76 +01:45:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65613_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 65613_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:27:15.17 +06:26:11.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)
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Considering the candidate 65614_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 65614_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:49:29.93 +08:30:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 3.029 3854723321275167360 147.37549419491 +08.51539991547 14.1838 13.6373 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.029#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65615_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 65615_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:21:53.73 +09:14:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 1.345 587703945892764544 140.47422000700 +09.24267967551 14.1797 13.5411 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.345#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65620_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 65620_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:31:40.95 +02:55:19.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)
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Considering the candidate 65622_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 65622_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:14:25.07 +07:54:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65625_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
Preparing report for the candidate 65625_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
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Considering the candidate 65627_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 65627_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:36:24.79 +02:47:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65629_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 65629_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:34:05.51 +02:30:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 0.657 3850580292742270976 143.52313435863 +02.51468784445 11.9733 11.4748 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.657#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66634_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 66634_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:51:27.36 +08:48:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66821_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 66821_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:10:35.90 +07:33:58.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66992_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 66992_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:04:12.99 +06:41:47.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67100_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
Preparing report for the candidate 67100_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
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Considering the candidate 67113_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 67113_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:10:45.09 +06:21:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 68013_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 68013_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:14:28.56 +07:47:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 68989_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 68989_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:34:54.68 +07:47:51.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69076_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 69076_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:11:56.00 +09:43:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69167_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 69167_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:14:28.10 +08:28:37.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69280_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
Preparing report for the candidate 69280_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
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Considering the candidate 69322_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 69322_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:15:11.36 +05:32:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 2.760 579799801614024064 138.79797210307 +05.53515478454 14.0806 13.2642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.760#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 69360_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 69360_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:22:25.96 +06:08:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 1.870 585896834107952512 140.60860444512 +06.14721673870 14.1711 13.7014 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.870#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 69436_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 69436_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:08:39.03 +05:16:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 1.122 580118316388363648 137.16293343062 +05.27964216446 14.3288 13.8655 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.122#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 69440_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 69440_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:19:43.41 +10:03:51.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69599_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 69599_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:15:54.09 +08:13:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69672_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 69672_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:16:00.60 +06:16:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 1.731 586616601907314048 139.00291915704 +06.27834350238 14.3839 13.9522 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.731#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 69948_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
Preparing report for the candidate 69948_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
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Considering the candidate 69962_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 69962_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:30:01.03 +02:06:30.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 1.877 3844548994722734208 142.50480059291 +02.10844131409 14.5697 14.0689 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.877#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70153_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 70153_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:19:44.99 +02:36:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 2.029 3845201967190611072 139.93801162168 +02.60791768226 14.4407 13.8459 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.029#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70264_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 70264_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:27:33.89 +06:20:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 3.808 586055713538484480 141.89201457569 +06.33419858597 14.7104 14.0452 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.808#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70441_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 70441_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:05:39.04 +05:31:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.62, MAG_FAINT_SEARCH_LIMIT=15.60)GAIADR2_OUTPUT=# 2.491 580369859737561216 136.41310209490 +05.53226612539 14.6647 14.1418 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.491#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70459_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 70459_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:09:25.94 +09:36:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 1.649 591294504191927680 137.35850867574 +09.60589917704 14.5709 14.0224 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.649#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70516_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 70516_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:07:36.22 +06:18:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 1.658 580811421030816000 136.90101229475 +06.30227164485 14.9825 14.4470 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.658#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70604_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 70604_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:09:49.21 +10:06:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.93, MAG_FAINT_SEARCH_LIMIT=15.91)GAIADR2_OUTPUT=# 1.582 591737852191628928 137.45520815446 +10.10417574278 14.9860 14.4568 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.582#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70753_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 70753_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:07:52.61 +08:42:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.89, MAG_FAINT_SEARCH_LIMIT=15.87)GAIADR2_OUTPUT=# 1.542 590379955331423360 136.96962276617 +08.70351413769 14.6713 13.8328 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70755_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 70755_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:12:23.09 +09:42:25.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.76, MAG_FAINT_SEARCH_LIMIT=15.74)
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Considering the candidate 70818_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 70818_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:02:11.09 +04:56:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.93, MAG_FAINT_SEARCH_LIMIT=15.91)GAIADR2_OUTPUT=# 0.801 580231359927791872 135.54633340061 +04.93865662675 14.8939 14.3803 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.801#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70830_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 70830_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:12:40.69 +09:16:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.94, MAG_FAINT_SEARCH_LIMIT=15.92)GAIADR2_OUTPUT=# 2.926 590464033611078144 138.17032597763 +09.27586311572 14.8143 14.5513 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.926#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70842_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 70842_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:11:57.44 +09:49:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)GAIADR2_OUTPUT=# 1.666 591670094787630336 137.98940140519 +09.82123668700 14.7465 14.2226 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.666#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70926_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 70926_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:24:54.01 +09:58:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.72, MAG_FAINT_SEARCH_LIMIT=15.70)GAIADR2_OUTPUT=# 1.519 589257663197126528 141.22534406115 +09.98082683520 14.8479 14.2942 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.519#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70931_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 70931_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:20:42.76 +09:19:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.64, MAG_FAINT_SEARCH_LIMIT=15.62)GAIADR2_OUTPUT=# 1.864 590687990385980416 140.17868379581 +09.32088406103 14.7728 14.1977 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70972_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 70972_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:11:00.49 +01:59:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)GAIADR2_OUTPUT=# 1.817 3843794862889708416 137.75229674867 +01.99561979841 15.0569 14.4091 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.817#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70998_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 70998_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:15:40.18 +07:59:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)GAIADR2_OUTPUT=# 2.784 587120006434228224 138.91811840599 +07.99482742698 14.9591 14.4658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.784#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71092_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 71092_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:15:43.57 +01:52:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71105_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 71105_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:50:05.59 +05:17:44.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 1.420 3849953815927656192 147.52308887158 +05.29532781945 14.6371 14.1086 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71145_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 71145_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:15:44.84 +06:04:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.94, MAG_FAINT_SEARCH_LIMIT=15.92)GAIADR2_OUTPUT=# 1.869 580605984155075328 138.93727910971 +06.07557576802 15.0249 14.2211 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.869#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71248_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 71248_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks
**** FOUND 09:41:50.85 +02:00:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.65, MAG_FAINT_SEARCH_LIMIT=15.63)GAIADR2_OUTPUT=# 0.876 3847347286175297920 145.46211078301 +02.00397745371 14.8830 14.3756 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.876#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71271_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
Preparing report for the candidate 71271_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
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Considering the candidate 71336_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143
The candidate 71336_fd_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143 did not pass the final checks