This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS
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 08.2766* 13 28 22.37 -22 08 29.8 12.7 U Vir 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,2461138.7766,12.70,0.05,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 20260408.2766 12.70CV 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 08.2766* 13 17 34.54 -21 56 34.0 13.8 U Vir 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,2461138.7766,13.78,0.05,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 20260408.2766 13.78CV 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
NSV 6170,2461138.7766,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 6170 20260408.2766 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J133537-2955.2,2461138.7766,11.62,0.05,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
ASAS J133537-2955.2 20260408.2766 11.62CV 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
ASAS J132439-2431.5,2461138.7766,11.38,0.05,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
ASAS J132439-2431.5 20260408.2766 11.38CV 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: 2461118.83151337 19.03.2026 07:57:12.755 /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
First image: 2461118.83151337 19.03.2026 07:57:12.755 /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
Last image: 2461138.77692196 08.04.2026 06:38:36.057 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.18
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): 4892
Objects passed selection criteria: 4890
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 4637.75
Average stars matched: 4523.75 (97.5419 %)
Memory usage VmPeak: 111256 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 Wed Apr 8 01:40:37 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: 2461118.83151337 19.03.2026 07:57:12.755 /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
First image: 2461118.83151337 19.03.2026 07:57:12.755 /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
Last image: 2461138.77692196 08.04.2026 06:38:36.057 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 73
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.86
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: 14 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): 31117
Objects passed selection criteria: 31063
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 28381.5
Average stars matched: 27382.5 (96.4801 %)
Memory usage VmPeak: 135692 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 Wed Apr 8 01:41:33 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
SExtractor catalog cache: saved Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits.cat to cache
SExtractor catalog cache: saved Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.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-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.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: 2461138.77636676
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-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits exists and is non-empty
Saving wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits to local_wcs_cache/
'wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits' -> 'local_wcs_cache/wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits'
wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits exists and is non-empty
Saving wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits to local_wcs_cache/
'wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits' -> 'local_wcs_cache/wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits'
wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits exists and is non-empty
Saving wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits to local_wcs_cache/
'wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits' -> 'local_wcs_cache/wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits'
wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits exists and is non-empty
Saving wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits to local_wcs_cache/
'wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits' -> 'local_wcs_cache/wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.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 13:26:24.609 -25:59:56.92
Second-epoch image center 13:26:11.260 -26:00:41.01
Angular distance between the image centers 0.0515 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 13:26:24.609 -25:59:56.92
Second-epoch image center 13:26:09.932 -26:01:00.59
Angular distance between the image centers 0.0577 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 13:26:11.260 -26:00:41.01
Second-epoch second image center 13:26:09.932 -26:01:00.59
Angular distance between the image centers 0.00737 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-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits &> /tmp/tmp.a1kc5jane1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits &> /tmp/tmp.7nzRK6Kl3s
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits &> /tmp/tmp.h8BFCd5wF2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits &> /tmp/tmp.mLLtcsmk16
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.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-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits and wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.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-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits and wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits.cat
Found non-empty wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits and wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits.cat
The reference image (wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits) and catalog (wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits.cat) found
'wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits.cat' -> 'wcsmag.cat'
Read 6454 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 192.4095 to 210.5380 deg, Dec -31.2848 to -20.5370 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 192.4095 to 210.5380 deg, Dec -31.2848 to -20.5370 deg
Loaded 6707 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): 4838 out of 4959 total matches.
Matched with Tycho-2 4959 out of 6454 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.777933
a=0.000000 b=1.000000 c=22.777933
From vast_summary.log: estimated ref. image limiting mag.: -8.18
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.60
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.60
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
2.4 pix Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits
3.4 pix fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits
3.4 pix fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
Limiting magnitude estimates:
14.6 mag. Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
14.6 mag. Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits
14.2 mag. fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits
14.2 mag. fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 11.6 (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.a1kc5jane1 (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_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.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-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits' -> 'wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
WCS_IMAGE_NAME=wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
WCS-calibrated image found: wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
Checking if the catalog wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits.cat corresponding to the image wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits alredy exist and is non-empty...
Catalog wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits.cat corresponding to the image wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
WCS catalog name: wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=400, passed=6454
Got 6454 stars (including 6044 good ones) from the SExtractor catalog wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits.cat
util/solve_plate_with_UCAC5 got 6454 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 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 963 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: 963 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 6381 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 6381 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 6381 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits -region wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.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.7nzRK6Kl3s (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_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.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-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits' -> 'wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits
WCS_IMAGE_NAME=wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits
WCS-calibrated image found: wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits
Checking if the catalog wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits.cat corresponding to the image wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits alredy exist and is non-empty...
Catalog wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits.cat corresponding to the image wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits
WCS catalog name: wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=400, passed=6442
Got 6442 stars (including 6028 good ones) from the SExtractor catalog wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits.cat
util/solve_plate_with_UCAC5 got 6442 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 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 964 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: 964 matched stars entering correct_measured_positions(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 6362 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 6363 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 6363 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits -region wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.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.h8BFCd5wF2 (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_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.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_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits
WCS_IMAGE_NAME=wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits
WCS-calibrated image found: wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits
Checking if the catalog wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits.cat corresponding to the image wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits.cat corresponding to the image wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits
WCS catalog name: wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=483, passed=5739
Got 5739 stars (including 5252 good ones) from the SExtractor catalog wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits.cat
util/solve_plate_with_UCAC5 got 5739 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 957 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: 957 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 5626 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 5627 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
WARNING: Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 5627 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits -region wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.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.mLLtcsmk16 (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_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.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_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
WCS_IMAGE_NAME=wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
WCS-calibrated image found: wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
Checking if the catalog wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits.cat corresponding to the image wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits.cat corresponding to the image wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
WCS catalog name: wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=487, passed=5731
Got 5731 stars (including 5242 good ones) from the SExtractor catalog wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits.cat
util/solve_plate_with_UCAC5 got 5731 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 956 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: 956 matched stars entering correct_measured_positions(), 950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 5629 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 5628 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
WARNING: Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 5628 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits -region wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.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-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits'
Saving fully-calibrated image wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits'
Saving fully-calibrated image wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits'
Saving fully-calibrated image wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits'
Preparing the HTML report for the field Hya-13-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20274.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 20274_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 20274_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:24:39.05 -24:31:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 1.961 6193435444622762240 201.16274291733 -24.52534504181 9.9287 8.4309 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.961#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-13-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-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
SExtractor catalog cache: saved Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits.cat to cache
SExtractor catalog cache: saved Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.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-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
Creating symlink local_wcs_cache/wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.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-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits exists and is non-empty
wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits exists and is non-empty
wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits exists and is non-empty
wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.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 13:26:24.609 -25:59:56.92
Second-epoch image center 13:26:11.260 -26:00:41.01
Angular distance between the image centers 0.0515 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 13:26:24.609 -25:59:56.92
Second-epoch image center 13:26:09.932 -26:01:00.59
Angular distance between the image centers 0.0577 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 13:26:11.260 -26:00:41.01
Second-epoch second image center 13:26:09.932 -26:01:00.59
Angular distance between the image centers 0.00737 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-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits &> /tmp/tmp.cgvx1QfmiW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits &> /tmp/tmp.UZVHu2dTQq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits &> /tmp/tmp.4P0Ahpi7pJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits &> /tmp/tmp.0ioXoQwcAp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.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-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits and wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.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-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits and wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits.cat
Found non-empty wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits and wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits.cat
The reference image (wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits) and catalog (wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits.cat) found
'wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits.cat' -> 'wcsmag.cat'
Read 40681 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 192.4095 to 210.5978 deg, Dec -31.2847 to -20.4442 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 192.4095 to 210.5978 deg, Dec -31.2847 to -20.4442 deg
Loaded 6790 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): 5287 out of 5690 total matches.
Matched with Tycho-2 5690 out of 40681 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.603442
a=0.000000 b=1.000000 c=22.603442
From vast_summary.log: estimated ref. image limiting mag.: -7.86
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.74
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.74
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 42 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
2.3 pix Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits
2.9 pix fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits
2.9 pix fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
Limiting magnitude estimates:
14.7 mag. Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
14.7 mag. Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits
14.4 mag. fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits
14.4 mag. fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 13.8 (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.cgvx1QfmiW (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_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.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-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits' -> 'wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
WCS_IMAGE_NAME=wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
WCS-calibrated image found: wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
Checking if the catalog wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits.cat corresponding to the image wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits alredy exist and is non-empty...
Catalog wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits.cat corresponding to the image wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
WCS catalog name: wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=1754, passed=40677
Got 40677 stars (including 38867 good ones) from the SExtractor catalog wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits.cat
util/solve_plate_with_UCAC5 got 40677 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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 962 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: 962 matched stars entering correct_measured_positions(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 40163 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 40165 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 40165 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits -region wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.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.UZVHu2dTQq (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_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.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-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits' -> 'wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits
WCS_IMAGE_NAME=wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits
WCS-calibrated image found: wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits
Checking if the catalog wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits.cat corresponding to the image wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits alredy exist and is non-empty...
Catalog wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits.cat corresponding to the image wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits
WCS catalog name: wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1755, passed=40890
Got 40890 stars (including 39093 good ones) from the SExtractor catalog wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits.cat
util/solve_plate_with_UCAC5 got 40890 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 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 964 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: 964 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 40374 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
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 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 40374 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 40373 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits -region wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.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.4P0Ahpi7pJ (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_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.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_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits
WCS_IMAGE_NAME=wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits
WCS-calibrated image found: wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits
Checking if the catalog wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits.cat corresponding to the image wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits.cat corresponding to the image wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits
WCS catalog name: wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=2486, passed=29840
Got 29840 stars (including 27338 good ones) from the SExtractor catalog wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits.cat
util/solve_plate_with_UCAC5 got 29840 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 955 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: 955 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 29337 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 29335 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
WARNING: Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 29335 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits -region wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.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.0ioXoQwcAp (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_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.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_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
WCS_IMAGE_NAME=wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
WCS-calibrated image found: wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
Checking if the catalog wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits.cat corresponding to the image wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits.cat corresponding to the image wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
WCS catalog name: wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=2429, passed=30088
Got 30088 stars (including 27633 good ones) from the SExtractor catalog wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits.cat
util/solve_plate_with_UCAC5 got 30088 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 955 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: 955 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 29501 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
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 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 29502 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
WARNING: Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 29501 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits -region wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.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-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.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_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/wcs_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits
Saving fully-calibrated image wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.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_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/wcs_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits
Saving fully-calibrated image wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.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_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-37-48_20.00sec_-4.90C_LIGHT_0094.fits
Saving fully-calibrated image wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.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_2026-04-08_CI_Hya-13-Q2b1x1_013921_TTUQ2b1x1_11172_NR84nLFS/wcs_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095.fits
Preparing the HTML report for the field Hya-13-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52630.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52632.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52633.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52833.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52992.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52994.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53009.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53011.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53016.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53040.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53042.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53059.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53060.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53063.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53069.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53073.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53074.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53078.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53082.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53087.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53088.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53089.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53096.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53099.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53116.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53126.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53141.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53152.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53163.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53167.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53174.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53184.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53219.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out05349.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40569.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52773.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53008.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52630_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 52630_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:37:35.26 -29:34:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 3.095 6175832774562288640 204.39656929589 -29.57080635505 13.3162 12.7214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.095#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52632_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 52632_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:34:03.69 -27:44:38.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52633_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 52633_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:03:51.08 -26:08:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 2.814 6187737569209334144 195.96347351897 -26.13927968689 14.0120 13.8677 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.814#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52642_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 52642_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 12:57:29.86 -24:25:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52773_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
Preparing report for the candidate 52773_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
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Considering the candidate 52796_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 52796_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:16:59.45 -22:01:06.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52833_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 52833_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:00:10.36 -23:08:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 0.511 3498941600708315264 195.04329163805 -23.14636127360 13.5118 12.9226 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.511#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52901_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 52901_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:26:09.50 -22:10:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52992_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 52992_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:09:34.40 -22:25:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 0.918 3504663802816545536 197.39310646728 -22.42945064349 13.8986 13.3990 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.918#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52994_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 52994_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:29:45.01 -22:22:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 4.106 6195249089052923648 202.43873861875 -22.37711304332 13.4932 12.5598 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.106#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53002_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
Preparing report for the candidate 53002_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
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Considering the candidate 53008_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
Preparing report for the candidate 53008_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
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Considering the candidate 53009_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 53009_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:02:13.61 -22:23:51.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)
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Considering the candidate 53011_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 53011_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:04:46.75 -22:34:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.08, MAG_FAINT_SEARCH_LIMIT=15.06)GAIADR2_OUTPUT=# 0.598 3505068079498228608 196.19489302742 -22.58055378541 13.9741 13.4528 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.598#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53016_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 53016_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 12:56:15.25 -25:33:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 1.529 3497494128010358272 194.06310123669 -25.55843351723 13.9030 13.3250 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.529#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53040_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 53040_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:01:02.23 -24:01:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 1.496 3498110988392979072 195.25929502594 -24.02130446418 14.1544 13.5725 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.496#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53042_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 53042_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 12:57:29.23 -23:24:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 1.598 3498952870702456960 194.37172372737 -23.40896718424 14.0214 13.4937 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.598#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53059_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 53059_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:06:27.33 -21:48:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 1.959 3505133019403811712 196.61381115138 -21.80284788204 14.1296 13.5136 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.959#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53060_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 53060_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 12:59:05.48 -22:27:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 1.221 3505214933020092288 194.77280011774 -22.45289326676 14.1853 13.6608 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.221#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53063_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 53063_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:06:08.47 -23:36:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 1.184 3504117379897327616 196.53505817396 -23.61069428799 14.1723 13.4962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.184#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53069_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 53069_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:06:03.66 -24:32:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 1.118 3497811646352391040 196.51553777868 -24.54708304624 14.1692 13.4454 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.118#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53073_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 53073_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:01:58.56 -23:51:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 1.777 3498137617190239872 195.49388404632 -23.85076780655 13.9114 13.3299 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.777#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53074_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 53074_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:04:07.80 -23:24:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 0.769 3504161772679312384 196.03272231515 -23.41654816225 14.0586 13.5349 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.769#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53078_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 53078_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:03:25.72 -22:02:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.17, MAG_FAINT_SEARCH_LIMIT=15.15)GAIADR2_OUTPUT=# 0.093 3505151882900052096 195.85713887768 -22.04494305784 14.0899 13.5024 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.093#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53082_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 53082_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 12:59:40.13 -22:16:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 0.247 3505224519387114752 194.91713502409 -22.27239881841 14.0806 13.5622 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.247#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53087_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 53087_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:06:48.08 -22:40:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 1.372 3504304056355850624 196.69993557157 -22.67785262184 14.0563 13.3683 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.372#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53088_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 53088_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:12:18.72 -22:00:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 0.889 3504694314264411520 198.07815878415 -22.00538494202 14.1185 13.4277 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53089_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 53089_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 12:57:28.41 -22:41:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 0.193 3499211702611632384 194.36839898669 -22.69882673962 14.1545 13.4623 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.193#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53096_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 53096_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 12:57:10.03 -24:41:40.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 1.564 3497978497241875200 194.29207308751 -24.69499020444 14.0895 13.6098 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.564#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53099_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 53099_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:17:09.79 -25:02:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 1.272 6192976261079442048 199.29053149593 -25.04290197749 13.4203 12.3122 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.272#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53116_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 53116_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:08:40.32 -25:23:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 0.850 6187848104487621376 197.16821527832 -25.38864395591 14.1361 13.6018 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53126_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 53126_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:06:33.38 -23:39:50.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 1.563 3503928676214370048 196.63895756036 -23.66444630593 14.4616 13.9200 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.563#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53141_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 53141_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:20:32.24 -22:58:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 0.528 6194408306255114368 200.13417915885 -22.97649032818 14.3919 13.7512 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.528#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53152_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 53152_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:08:49.61 -24:54:39.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)
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Considering the candidate 53163_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 53163_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:08:37.46 -24:10:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 0.757 3503840333031051392 197.15612503239 -24.16884579288 14.4246 13.9482 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.757#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53167_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 53167_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:05:32.65 -24:22:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 1.280 3497864010593599104 196.38614176795 -24.37434365594 14.2227 13.6038 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.280#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53174_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 53174_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:15:26.21 -22:41:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 1.198 3504410739048134144 198.85899663027 -22.69713069098 14.3092 13.4126 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.198#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53184_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 53184_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:21:17.82 -22:03:06.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)
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Considering the candidate 53219_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 53219_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks
**** FOUND 13:22:16.08 -23:23:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 1.467 6194333505104733056 200.56693198660 -23.39518054060 14.1670 13.5565 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.467#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 05349_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
Preparing report for the candidate 05349_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
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Considering the candidate 40569_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
Preparing report for the candidate 40569_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
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Considering the candidate 26002_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095
The candidate 26002_fd_Hya-13-Q2b1x1_2026-04-08_01-38-36_20.00sec_-4.90C_LIGHT_0095 did not pass the final checks