This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6986,13.55,0.05,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
target 20260410.1986 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6986,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1986 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6986,12.87,0.05,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
target 20260410.1986 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J126.1644-03.3227,2461140.6986,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J126.1644-03.3227 20260410.1986 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6986,12.65,0.05,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
target 20260410.1986 12.65CV 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: 2461119.65034514 20.03.2026 03:36:19.820 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
First image: 2461119.65034514 20.03.2026 03:36:19.820 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
Last image: 2461140.69899981 10.04.2026 04:46:23.584 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 8
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.80
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: 8 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): 11850
Objects passed selection criteria: 11828
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: 10497.2
Average stars matched: 10299 (98.1114 %)
Memory usage VmPeak: 118196 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 10 00:13:10 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: 2461119.65034514 20.03.2026 03:36:19.820 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
First image: 2461119.65034514 20.03.2026 03:36:19.820 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
Last image: 2461140.69899981 10.04.2026 04:46:23.584 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 55
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.52
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: 40 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): 66858
Objects passed selection criteria: 66747
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 55927.5
Average stars matched: 54021.5 (96.592 %)
Memory usage VmPeak: 171408 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 10 00:14:50 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-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
SExtractor catalog cache: saved Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits.cat to cache
SExtractor catalog cache: saved Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.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-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.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: 2461140.69819155
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-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits exists and is non-empty
Saving wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits to local_wcs_cache/
'wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits' -> 'local_wcs_cache/wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits'
wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits exists and is non-empty
Saving wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits to local_wcs_cache/
'wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits' -> 'local_wcs_cache/wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits'
wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits exists and is non-empty
Saving wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits to local_wcs_cache/
'wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits' -> 'local_wcs_cache/wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits'
wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits exists and is non-empty
Saving wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits to local_wcs_cache/
'wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits' -> 'local_wcs_cache/wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.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 08:34:25.148 -01:59:29.07
Second-epoch image center 08:34:22.048 -02:01:41.27
Angular distance between the image centers 0.0389 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 08:34:25.148 -01:59:29.07
Second-epoch image center 08:34:25.144 -02:01:18.82
Angular distance between the image centers 0.0305 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 08:34:22.048 -02:01:41.27
Second-epoch second image center 08:34:25.144 -02:01:18.82
Angular distance between the image centers 0.01432 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-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits &> /tmp/tmp.nOt8nzMiEH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits &> /tmp/tmp.itAs1Tb5Jm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits &> /tmp/tmp.G1Yvv6iV15
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits &> /tmp/tmp.oelbiFics3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.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-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits and wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.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-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits and wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits.cat
Found non-empty wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits and wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits.cat
The reference image (wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits) and catalog (wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits.cat) found
'wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits.cat' -> 'wcsmag.cat'
Read 17362 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 120.6326 to 136.5134 deg, Dec -7.3344 to +3.3888 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 120.6326 to 136.5134 deg, Dec -7.3344 to 3.3888 deg
Loaded 10338 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): 8455 out of 8861 total matches.
Matched with Tycho-2 8861 out of 17362 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.920054
a=0.000000 b=1.000000 c=22.920054
From vast_summary.log: estimated ref. image limiting mag.: -7.80
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.12
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.12
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.6 pix Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
2.6 pix Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits
4.2 pix fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits
4.2 pix fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
Limiting magnitude estimates:
15.1 mag. Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
15.1 mag. Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits
14.5 mag. fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits
14.5 mag. fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.nOt8nzMiEH (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_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.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-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits' -> 'wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
WCS_IMAGE_NAME=wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
WCS-calibrated image found: wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
Checking if the catalog wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits.cat corresponding to the image wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits alredy exist and is non-empty...
Catalog wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits.cat corresponding to the image wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
WCS catalog name: wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1075, passed=17362
Got 17362 stars (including 16274 good ones) from the SExtractor catalog wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits.cat
util/solve_plate_with_UCAC5 got 17362 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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 16489 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 16486 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 16486 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits -region wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.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.itAs1Tb5Jm (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_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.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-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits' -> 'wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits
WCS_IMAGE_NAME=wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits
WCS-calibrated image found: wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits
Checking if the catalog wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits.cat corresponding to the image wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits alredy exist and is non-empty...
Catalog wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits.cat corresponding to the image wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits
WCS catalog name: wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1136, passed=17334
Got 17334 stars (including 16184 good ones) from the SExtractor catalog wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits.cat
util/solve_plate_with_UCAC5 got 17334 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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 16477 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 16477 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 16477 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits -region wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.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.G1Yvv6iV15 (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_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.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_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits
WCS_IMAGE_NAME=wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits
WCS-calibrated image found: wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits
Checking if the catalog wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits.cat corresponding to the image wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits.cat corresponding to the image wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits
WCS catalog name: wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1549, passed=11382
Got 11382 stars (including 9831 good ones) from the SExtractor catalog wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits.cat
util/solve_plate_with_UCAC5 got 11382 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (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 0.010409 (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 413 to 468 (Dec -7.4 to 3.3)
Done reading UCAC5 zone files...
Matched 917 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 900 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.88"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 11153 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.95"
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 413 to 468 (Dec -7.4 to 3.3)
Done reading UCAC5 zone files...
Matched 917 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 11154 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.96"
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 11154 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.02"
Excluding outliers - 915 stars left (next iteration limit 1006)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits -region wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.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.oelbiFics3 (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_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.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_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
WCS_IMAGE_NAME=wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
WCS-calibrated image found: wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
Checking if the catalog wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits.cat corresponding to the image wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits.cat corresponding to the image wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
WCS catalog name: wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1515, passed=11364
Got 11364 stars (including 9844 good ones) from the SExtractor catalog wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits.cat
util/solve_plate_with_UCAC5 got 11364 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (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 0.010409 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 916 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 894 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.90"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 11051 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.95"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 916 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 11053 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.96"
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 11053 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.03"
Excluding outliers - 915 stars left (next iteration limit 1006)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits -region wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.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-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits'
Saving fully-calibrated image wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits'
Saving fully-calibrated image wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits'
Saving fully-calibrated image wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits'
Preparing the HTML report for the field Hya-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out08646.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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20601_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
The candidate 20601_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075 did not pass the final checks
**** FOUND 08:30:44.62 -06:15:08.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20656_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
The candidate 20656_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075 did not pass the final checks
**** FOUND 08:59:30.41 -06:00:28.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20667_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
The candidate 20667_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075 did not pass the final checks
**** FOUND 08:54:15.16 -05:55:30.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08646_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
The candidate 08646_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075 did not pass the final checks
**** FOUND 08:44:21.94 -02:20:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 4.311 3072256524203069184 131.09123178767 -02.33401137237 11.7061 11.3909 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.311#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: 1s
Prepared the HTML report for the field Hya-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
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-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
SExtractor catalog cache: saved Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits.cat to cache
SExtractor catalog cache: saved Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.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-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
Creating symlink local_wcs_cache/wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.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-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits exists and is non-empty
wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits exists and is non-empty
wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits exists and is non-empty
wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.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 08:34:25.148 -01:59:29.07
Second-epoch image center 08:34:22.048 -02:01:41.27
Angular distance between the image centers 0.0389 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 08:34:25.148 -01:59:29.07
Second-epoch image center 08:34:25.144 -02:01:18.82
Angular distance between the image centers 0.0305 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 08:34:22.048 -02:01:41.27
Second-epoch second image center 08:34:25.144 -02:01:18.82
Angular distance between the image centers 0.01432 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-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits &> /tmp/tmp.IxMuHgsS58
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits &> /tmp/tmp.83ff9kvPoa
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits &> /tmp/tmp.OQM1UmWqyw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits &> /tmp/tmp.5lSj0huvNx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.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-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits and wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.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-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits and wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits.cat
Found non-empty wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits and wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits.cat
The reference image (wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits) and catalog (wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits.cat) found
'wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits.cat' -> 'wcsmag.cat'
Read 91055 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 120.6321 to 136.5265 deg, Dec -7.3344 to +3.3893 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 120.6321 to 136.5265 deg, Dec -7.3344 to 3.3893 deg
Loaded 10343 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): 7637 out of 8952 total matches.
Matched with Tycho-2 8952 out of 91055 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.795363
a=0.000000 b=1.000000 c=22.795363
From vast_summary.log: estimated ref. image limiting mag.: -7.52
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.28
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.28
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 29 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
2.4 pix Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits
3.9 pix fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits
3.9 pix fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
Limiting magnitude estimates:
15.3 mag. Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
15.3 mag. Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits
14.6 mag. fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits
14.6 mag. fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
All-image limiting magnitude estimate: 14.6 (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.IxMuHgsS58 (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_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.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-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits' -> 'wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
WCS_IMAGE_NAME=wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
WCS-calibrated image found: wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
Checking if the catalog wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits.cat corresponding to the image wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits alredy exist and is non-empty...
Catalog wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits.cat corresponding to the image wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
WCS catalog name: wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=7506, passed=91044
Got 91044 stars (including 83450 good ones) from the SExtractor catalog wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits.cat
util/solve_plate_with_UCAC5 got 91044 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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 88159 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 88159 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 88158 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits -region wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.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.83ff9kvPoa (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_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.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-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits' -> 'wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits
WCS_IMAGE_NAME=wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits
WCS-calibrated image found: wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits
Checking if the catalog wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits.cat corresponding to the image wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits alredy exist and is non-empty...
Catalog wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits.cat corresponding to the image wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits
WCS catalog name: wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=7991, passed=93852
Got 93852 stars (including 85771 good ones) from the SExtractor catalog wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits.cat
util/solve_plate_with_UCAC5 got 93852 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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 90418 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 90418 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 90418 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits -region wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.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.OQM1UmWqyw (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_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.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_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits
WCS_IMAGE_NAME=wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits
WCS-calibrated image found: wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits
Checking if the catalog wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits.cat corresponding to the image wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits.cat corresponding to the image wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits
WCS catalog name: wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=9061, passed=50870
Got 50870 stars (including 41790 good ones) from the SExtractor catalog wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits.cat
util/solve_plate_with_UCAC5 got 50870 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (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 0.010409 (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 413 to 468 (Dec -7.4 to 3.3)
Done reading UCAC5 zone files...
Matched 914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 892 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.85"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 49547 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.85"
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 413 to 468 (Dec -7.4 to 3.3)
Done reading UCAC5 zone files...
Matched 914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 49546 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.85"
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 49546 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.91"
Excluding outliers - 912 stars left (next iteration limit 1003)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits -region wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.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.5lSj0huvNx (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_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.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_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
WCS_IMAGE_NAME=wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
WCS-calibrated image found: wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
Checking if the catalog wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits.cat corresponding to the image wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits.cat corresponding to the image wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
WCS catalog name: wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=8776, passed=50580
Got 50580 stars (including 41789 good ones) from the SExtractor catalog wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits.cat
util/solve_plate_with_UCAC5 got 50580 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (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 0.010409 (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 413 to 468 (Dec -7.4 to 3.3)
Done reading UCAC5 zone files...
Matched 912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 911 matched stars entering correct_measured_positions(), 895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.86"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 911 matched stars entering correct_measured_positions(), 49280 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.85"
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 413 to 468 (Dec -7.4 to 3.3)
Done reading UCAC5 zone files...
Matched 912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 911 matched stars entering correct_measured_positions(), 49277 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.85"
Accuracy estimation diagnostic: 911 matched stars entering correct_measured_positions(), 49277 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.92"
Excluding outliers - 911 stars left (next iteration limit 1002)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits -region wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.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-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.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_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/wcs_Hya-03-Q2b1x1_2026-03-19_22-36-19_20.00sec_-14.90C_LIGHT_0106.fits
Saving fully-calibrated image wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.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_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/wcs_Hya-03-Q2b1x1_2026-03-19_22-37-03_20.00sec_-15.00C_LIGHT_0107.fits
Saving fully-calibrated image wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.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_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-45-13_20.00sec_-4.90C_LIGHT_0074.fits
Saving fully-calibrated image wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.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_2026-04-09_CI_Hya-03-Q2b1x1_234709_TTUQ2b1x1_26981_PYPu45cr/wcs_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075.fits
Preparing the HTML report for the field Hya-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out107718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107722.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107730.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107758.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107776.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107793.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108419.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out107755.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107756.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107801.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107805.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 19s
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 107718_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
The candidate 107718_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075 did not pass the final checks
**** FOUND 08:40:29.04 -01:03:00.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107722_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
The candidate 107722_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075 did not pass the final checks
**** FOUND 08:38:55.47 -02:22:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 4.138 3072396132116026880 129.73033664311 -02.37992034415 14.2392 13.7746 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.138#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107729_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
The candidate 107729_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075 did not pass the final checks
**** FOUND 08:48:16.65 -05:45:55.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107730_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
The candidate 107730_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075 did not pass the final checks
**** FOUND 08:31:47.28 -02:36:48.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107755_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
Preparing report for the candidate 107755_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107756_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
Preparing report for the candidate 107756_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107758_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
The candidate 107758_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075 did not pass the final checks
**** FOUND 08:16:55.21 -05:30:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 0.595 3064597227422301312 124.23008190851 -05.50785478269 12.8302 12.2502 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107776_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
The candidate 107776_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075 did not pass the final checks
**** FOUND 08:20:25.80 -02:12:40.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107788_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
The candidate 107788_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075 did not pass the final checks
**** FOUND 08:20:10.68 -05:20:47.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107791_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
Preparing report for the candidate 107791_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107793_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
The candidate 107793_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075 did not pass the final checks
**** FOUND 08:18:41.70 -04:33:22.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107798_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
The candidate 107798_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075 did not pass the final checks
**** FOUND 08:22:41.40 -04:03:02.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107801_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
Preparing report for the candidate 107801_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107805_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
Preparing report for the candidate 107805_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107816_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
The candidate 107816_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075 did not pass the final checks
**** FOUND 08:23:48.18 -01:32:47.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107977_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
The candidate 107977_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075 did not pass the final checks
**** FOUND 08:46:15.92 +01:35:56.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 108194_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
The candidate 108194_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075 did not pass the final checks
**** FOUND 08:39:20.02 -04:50:42.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 108236_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
The candidate 108236_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075 did not pass the final checks
**** FOUND 08:46:09.69 -00:16:14.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 108255_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
The candidate 108255_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075 did not pass the final checks
**** FOUND 08:41:25.61 -04:49:33.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 108419_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
The candidate 108419_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075 did not pass the final checks
**** FOUND 08:56:38.88 +00:22:25.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 3.211 3074541038783293824 134.16111654756 +00.37381778921 14.6982 14.2198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.211#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101379_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
The candidate 101379_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075 did not pass the final checks
**** FOUND 08:16:53.98 -04:48:31.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101493_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
The candidate 101493_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075 did not pass the final checks
**** FOUND 08:16:42.60 +00:00:35.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61063_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
The candidate 61063_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075 did not pass the final checks
**** FOUND 08:30:44.61 -06:15:08.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86898_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
The candidate 86898_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075 did not pass the final checks
**** FOUND 08:26:27.22 -03:59:14.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 88390_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
The candidate 88390_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075 did not pass the final checks
**** FOUND 08:24:34.79 -03:45:02.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 87542_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
The candidate 87542_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075 did not pass the final checks
**** FOUND 08:25:39.73 -03:54:18.9 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 81800_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
The candidate 81800_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075 did not pass the final checks
**** FOUND 08:24:36.51 -04:43:01.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77422_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
The candidate 77422_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075 did not pass the final checks
**** FOUND 08:20:17.11 -05:19:47.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07227_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075
The candidate 07227_fd_Hya-03-Q2b1x1_2026-04-09_23-46-23_20.00sec_-4.90C_LIGHT_0075 did not pass the final checks