This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.1939* 09 42 10.31 +04 40 24.8 13.6 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6939,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1939 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.1939* 09 32 09.62 +09 17 22.7 12.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461146.6939,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.1939 12.93CV 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
VARIABLE_NAME,2461146.6939,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.1939 14.24CV 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
VARIABLE_NAME,2461146.6939,14.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.1939 14.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.74633115 22.02.2026 05:54:33.011 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
First image: 2461093.74633115 22.02.2026 05:54:33.011 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Last image: 2461146.69417571 16.04.2026 04:39:26.781 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 0
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.65
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 8874
Objects passed selection criteria: 8831
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 6778.5
Average stars matched: 6248 (92.1738 %)
Memory usage VmPeak: 113708 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 15 23:55:19 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.74633115 22.02.2026 05:54:33.011 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
First image: 2461093.74633115 22.02.2026 05:54:33.011 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Last image: 2461146.69417571 16.04.2026 04:39:26.781 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 69
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.35
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: 22 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): 49731
Objects passed selection criteria: 49566
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 39981.5
Average stars matched: 36739.8 (91.8919 %)
Memory usage VmPeak: 145260 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 15 23:56:29 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
SExtractor catalog cache: saved Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat to cache
SExtractor catalog cache: saved Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.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: 2461146.69359090
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits exists and is non-empty
Saving wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits to local_wcs_cache/
'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits' -> 'local_wcs_cache/wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits'
wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits exists and is non-empty
Saving wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits to local_wcs_cache/
'wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits' -> 'local_wcs_cache/wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits'
wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits exists and is non-empty
Saving wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits to local_wcs_cache/
'wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits' -> 'local_wcs_cache/wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits'
wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits exists and is non-empty
Saving wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits to local_wcs_cache/
'wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits' -> 'local_wcs_cache/wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits (1st reference image)
verification OK: wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Image size: 937.5'x624.8' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 09:25:43.014 +06:00:02.92 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits (1st new image)
verification OK: wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits
Image size: 937.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 09:25:42.712 +05:57:36.49 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:25:43.014 +06:00:02.92
Second-epoch image center 09:25:42.712 +05:57:36.49
Angular distance between the image centers 0.0407 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits (2nd new image)
verification OK: wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
Image size: 937.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 09:25:45.756 +05:57:21.02 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:25:43.014 +06:00:02.92
Second-epoch image center 09:25:45.756 +05:57:21.02
Angular distance between the image centers 0.0464 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:25:42.712 +05:57:36.49
Second-epoch second image center 09:25:45.756 +05:57:21.02
Angular distance between the image centers 0.01333 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits &> /tmp/tmp.JXWj8Caodx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits &> /tmp/tmp.uK5a03ux5b
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits &> /tmp/tmp.JWQ3Md4hTF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits &> /tmp/tmp.LydThELyFj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
Found non-empty wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
The reference image (wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits) and catalog (wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat) found
'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat' -> 'wcsmag.cat'
Read 9705 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 133.2099 to 149.7640 deg, Dec +0.1004 to +11.7220 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 133.2099 to 149.7640 deg, Dec 0.1004 to 11.7220 deg
Loaded 6611 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4811 out of 5047 total matches.
Matched with Tycho-2 5047 out of 9705 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.925124
a=0.000000 b=1.000000 c=22.925124
From vast_summary.log: estimated ref. image limiting mag.: -7.65
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.28
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.28
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.5 pix Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
2.5 pix Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
2.5 pix fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits
2.5 pix fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
Limiting magnitude estimates:
15.3 mag. Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
15.3 mag. Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
15.0 mag. fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits
15.0 mag. fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.JXWj8Caodx (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_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits' -> 'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS-calibrated image found: wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Checking if the catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS catalog name: wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=629, passed=9705
Got 9705 stars (including 9071 good ones) from the SExtractor catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
util/solve_plate_with_UCAC5 got 9705 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 510 (Dec 0.1 to 11.7)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 9526 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 510 (Dec 0.1 to 11.7)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 9526 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 9526 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 939 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits -region wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.uK5a03ux5b (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_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits' -> 'wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS-calibrated image found: wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Checking if the catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS catalog name: wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=616, passed=9704
Got 9704 stars (including 9075 good ones) from the SExtractor catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat
util/solve_plate_with_UCAC5 got 9704 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 926 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 9534 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 9536 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 9537 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 937 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits -region wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.JWQ3Md4hTF (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_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.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_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits
Checking if the catalog wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits
WCS catalog name: wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=518, passed=8314
Got 8314 stars (including 7789 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits.cat
util/solve_plate_with_UCAC5 got 8314 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 8104 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
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 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 8104 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 8104 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits -region wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.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.LydThELyFj (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_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.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_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
Checking if the catalog wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
WCS catalog name: wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=500, passed=8376
Got 8376 stars (including 7871 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits.cat
util/solve_plate_with_UCAC5 got 8376 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 8184 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 8185 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 8182 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 944 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits -region wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits'
Saving fully-calibrated image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits'
Saving fully-calibrated image wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits'
Saving fully-calibrated image wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits'
Preparing the HTML report for the field Hya-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Hya-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
SExtractor catalog cache: saved Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat to cache
SExtractor catalog cache: saved Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Creating symlink local_wcs_cache/wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits exists and is non-empty
wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits exists and is non-empty
wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits exists and is non-empty
wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits (1st reference image)
verification OK: wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Image size: 937.5'x624.8' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 09:25:43.014 +06:00:02.92 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits (1st new image)
verification OK: wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits
Image size: 937.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 09:25:42.712 +05:57:36.49 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:25:43.014 +06:00:02.92
Second-epoch image center 09:25:42.712 +05:57:36.49
Angular distance between the image centers 0.0407 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits (2nd new image)
verification OK: wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
Image size: 937.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 09:25:45.756 +05:57:21.02 J2000 4789.000 3195.000
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# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:25:43.014 +06:00:02.92
Second-epoch image center 09:25:45.756 +05:57:21.02
Angular distance between the image centers 0.0464 deg.
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###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:25:42.712 +05:57:36.49
Second-epoch second image center 09:25:45.756 +05:57:21.02
Angular distance between the image centers 0.01333 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits &> /tmp/tmp.MkzAnJsiwE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits &> /tmp/tmp.kr1jQOZjVX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits &> /tmp/tmp.j4yNQbyRy1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits &> /tmp/tmp.dstndGV46Y
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
Found non-empty wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
The reference image (wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits) and catalog (wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat) found
'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat' -> 'wcsmag.cat'
Read 52265 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 133.1873 to 149.7640 deg, Dec +0.0999 to +11.7791 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 133.1873 to 149.7640 deg, Dec 0.0999 to 11.7791 deg
Loaded 6657 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4491 out of 5088 total matches.
Matched with Tycho-2 5088 out of 52265 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.799339
a=0.000000 b=1.000000 c=22.799339
From vast_summary.log: estimated ref. image limiting mag.: -7.35
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.45
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.45
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 38 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.3 pix Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
2.3 pix Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
2.2 pix fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits
2.2 pix fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
Limiting magnitude estimates:
15.4 mag. Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
15.4 mag. Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
15.3 mag. fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits
15.3 mag. fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 14.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.MkzAnJsiwE (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_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits' -> 'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS-calibrated image found: wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Checking if the catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS catalog name: wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=3222, passed=52238
Got 52238 stars (including 48939 good ones) from the SExtractor catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
util/solve_plate_with_UCAC5 got 52238 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 510 (Dec 0.1 to 11.8)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 51515 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 510 (Dec 0.1 to 11.8)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 51515 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 51515 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits -region wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.kr1jQOZjVX (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_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits' -> 'wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS-calibrated image found: wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Checking if the catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS catalog name: wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=3213, passed=52136
Got 52136 stars (including 48850 good ones) from the SExtractor catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat
util/solve_plate_with_UCAC5 got 52136 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 510 (Dec 0.1 to 11.8)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 51370 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 510 (Dec 0.1 to 11.8)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 51371 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 51371 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits -region wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.j4yNQbyRy1 (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_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.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_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits
Checking if the catalog wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits
WCS catalog name: wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=2394, passed=47668
Got 47668 stars (including 45213 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits.cat
util/solve_plate_with_UCAC5 got 47668 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 46512 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
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 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 46512 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 46512 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 940 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits -region wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.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.dstndGV46Y (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_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.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_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
Checking if the catalog wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
WCS catalog name: wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=2361, passed=47087
Got 47087 stars (including 44668 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits.cat
util/solve_plate_with_UCAC5 got 47087 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 46118 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 46119 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 46119 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 940 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits -region wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Saving fully-calibrated image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Saving fully-calibrated image wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.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_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-38-36_20.00sec_-4.90C_LIGHT_0144.fits
Saving fully-calibrated image wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.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_2026-04-15_CI_Hya-02-Q2b1x1_234851_TTUQ2b1x1_1478_R0m9DzpE/wcs_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145.fits
Preparing the HTML report for the field Hya-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out65385.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71737.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72522.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72666.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72842.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72984.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out65409.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70793.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71674.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
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Considering the candidate 65385_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 65385_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:42:06.72 +03:25:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.56, MAG_FAINT_SEARCH_LIMIT=15.54)GAIADR2_OUTPUT=# 0.914 3848075880131735808 145.52775798653 +03.42871718282 14.4040 13.8644 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.914#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65389_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 65389_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:39:00.92 +04:11:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.70, MAG_FAINT_SEARCH_LIMIT=15.68)GAIADR2_OUTPUT=# 1.665 3851223648778568832 144.75424534240 +04.18524019093 15.0435 14.4861 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.665#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65392_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 65392_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:11:20.66 +08:56:58.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65393_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 65393_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:32:53.97 +04:22:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65400_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 65400_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:19:45.02 +02:36:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65405_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 65405_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:25:50.25 +04:13:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65408_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 65408_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:31:40.87 +02:55:18.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65409_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
Preparing report for the candidate 65409_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
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Considering the candidate 65411_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 65411_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:14:25.14 +07:54:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65413_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 65413_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:42:41.00 +08:07:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65415_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 65415_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:36:24.83 +02:47:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65416_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 65416_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:34:05.47 +02:30:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67237_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 67237_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:10:45.10 +06:21:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67475_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
Preparing report for the candidate 67475_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
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Considering the candidate 68319_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 68319_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:12:01.84 +09:44:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 68336_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 68336_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:14:28.57 +07:47:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69638_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 69638_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:22:25.95 +06:08:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69686_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 69686_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:14:29.16 +02:20:21.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 69719_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 69719_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:11:25.08 +06:42:02.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70102_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 70102_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:14:28.09 +08:28:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70217_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 70217_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:11:12.65 +09:47:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70325_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 70325_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:15:54.16 +08:13:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70412_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 70412_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:11:56.04 +09:43:51.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70427_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 70427_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:19:43.49 +10:03:51.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70793_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
Preparing report for the candidate 70793_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
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Considering the candidate 71392_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 71392_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:30:01.04 +02:06:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71464_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 71464_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:22:42.08 +01:44:26.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71549_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 71549_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:09:26.07 +09:36:21.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71590_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 71590_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:17:25.73 +09:32:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71674_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
Preparing report for the candidate 71674_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
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Considering the candidate 71737_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 71737_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:16:03.97 +06:17:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.70, MAG_FAINT_SEARCH_LIMIT=15.68)GAIADR2_OUTPUT=# 2.482 586616631972157568 139.01720752604 +06.28541578637 15.0025 14.4881 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.482#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 72146_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 72146_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:12:40.72 +09:16:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72356_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 72356_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:16:52.51 +08:42:54.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72522_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 72522_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:16:27.84 +07:38:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.87, MAG_FAINT_SEARCH_LIMIT=15.85)GAIADR2_OUTPUT=# 1.665 587048194581040640 139.11646519887 +07.64111854052 14.9066 14.3958 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.665#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 72642_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 72642_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:32:29.19 +09:21:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72666_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 72666_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:36:48.94 +02:35:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.70, MAG_FAINT_SEARCH_LIMIT=15.68)GAIADR2_OUTPUT=# 0.432 3847594195254982528 144.20401391104 +02.59473506900 14.9899 14.4006 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.432#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 72842_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 72842_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:25:37.32 +01:44:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 1.986 3844477663905839232 141.40599433396 +01.73977325076 15.1562 14.6558 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.986#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 72984_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145
The candidate 72984_fd_Hya-02-Q2b1x1_2026-04-15_23-39-26_20.00sec_-5.00C_LIGHT_0145 did not pass the final checks