This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA
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 03.1151* 05 55 41.03 +23 15 21.3 11.6 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461133.6151,11.63,0.05,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 20260403.1151 11.63CV 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 03.1151* 05 26 53.39 +21 03 04.8 11.5 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461133.6151,11.47,0.05,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 20260403.1151 11.47CV 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 03.1151* 05 19 42.35 +26 04 09.9 12.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461133.6151,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260403.1151 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 03.1151* 05 35 04.78 +18 57 10.8 12.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461133.6151,12.92,0.05,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 20260403.1151 12.92CV 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 03.1151* 05 23 07.09 +18 37 43.5 12.7 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461133.6151,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260403.1151 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.62137122 11.02.2026 02:54:36.473 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
First image: 2461082.62137122 11.02.2026 02:54:36.473 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Last image: 2461133.61540271 03.04.2026 02:46:00.794 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.67
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): 17976
Objects passed selection criteria: 17876
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 11678.5
Average stars matched: 11022.8 (94.385 %)
Memory usage VmPeak: 123200 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 2 15:05:05 CDT 2026
VaST build number 1.0rc88-377-g075272b0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 2 21:49:28 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: 2461082.62137122 11.02.2026 02:54:36.473 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
First image: 2461082.62137122 11.02.2026 02:54:36.473 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Last image: 2461133.61540271 03.04.2026 02:46:00.794 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 91
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.29
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: 24 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): 132065
Objects passed selection criteria: 131749
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 91043.5
Average stars matched: 85287 (93.6772 %)
Memory usage VmPeak: 2027440 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 2 15:05:05 CDT 2026
VaST build number 1.0rc88-377-g075272b0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 2 21:51:41 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/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
SExtractor catalog cache: saved Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat to cache
SExtractor catalog cache: saved Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.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/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.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: 2461133.61475030
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits exists and is non-empty
Saving wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits to local_wcs_cache/
'wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits' -> 'local_wcs_cache/wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits'
wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits exists and is non-empty
Saving wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits to local_wcs_cache/
'wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits' -> 'local_wcs_cache/wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits'
wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits exists and is non-empty
Saving wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits to local_wcs_cache/
'wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits' -> 'local_wcs_cache/wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits'
wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits exists and is non-empty
Saving wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits to local_wcs_cache/
'wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits' -> 'local_wcs_cache/wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:32:19.616 +22:00:01.42
Second-epoch image center 05:32:18.221 +21:59:52.64
Angular distance between the image centers 0.0059 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:32:19.616 +22:00:01.42
Second-epoch image center 05:32:18.908 +22:00:21.48
Angular distance between the image centers 0.0062 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 05:32:18.221 +21:59:52.64
Second-epoch second image center 05:32:18.908 +22:00:21.48
Angular distance between the image centers 0.00844 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/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits &> /tmp/tmp.0UvR9igR8V
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits &> /tmp/tmp.3RBKaarG7r
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits &> /tmp/tmp.KKJA238PYH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits &> /tmp/tmp.AT7ViAsHW1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits and wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits and wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
Found non-empty wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits and wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
The reference image (wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits) and catalog (wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat) found
'wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat' -> 'wcsmag.cat'
Read 23525 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 74.1682 to 91.6910 deg, Dec +16.3328 to +27.3474 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 74.1682 to 91.6910 deg, Dec 16.3328 to 27.3474 deg
Loaded 12326 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): 9058 out of 10254 total matches.
Matched with Tycho-2 10254 out of 23525 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.945337
a=0.000000 b=1.000000 c=22.945337
From vast_summary.log: estimated ref. image limiting mag.: -7.67
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 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
2.3 pix Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
2.5 pix fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits
2.6 pix fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
Limiting magnitude estimates:
15.3 mag. Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
15.3 mag. Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
13.7 mag. fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits
13.5 mag. fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 10.8 (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.0UvR9igR8V (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits' -> 'wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WCS-calibrated image found: wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Checking if the catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WCS catalog name: wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2582, passed=23525
Got 23525 stars (including 20915 good ones) from the SExtractor catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
util/solve_plate_with_UCAC5 got 23525 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 927 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits -region wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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.3RBKaarG7r (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits' -> 'wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WCS-calibrated image found: wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
Checking if the catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WCS catalog name: wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2595, passed=23514
Got 23514 stars (including 20891 good ones) from the SExtractor catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat
util/solve_plate_with_UCAC5 got 23514 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.46"
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 926 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits -region wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.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.KKJA238PYH (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_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.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_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits
Checking if the catalog wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits
WCS catalog name: wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=428, passed=6220
Got 6220 stars (including 5785 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits.cat
util/solve_plate_with_UCAC5 got 6220 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.54"
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 930 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits -region wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.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.AT7ViAsHW1 (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_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.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_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
Checking if the catalog wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
WCS catalog name: wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=364, passed=5563
Got 5563 stars (including 5198 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits.cat
util/solve_plate_with_UCAC5 got 5563 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.56"
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 927 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits -region wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.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_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits'
Saving fully-calibrated image wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits'
Saving fully-calibrated image wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits'
Saving fully-calibrated image wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits'
Preparing the HTML report for the field Tau-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32149_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 32149_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:09:43.12 +23:02:03.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Tau-04-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/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
SExtractor catalog cache: saved Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat to cache
SExtractor catalog cache: saved Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Creating symlink local_wcs_cache/wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.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_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits exists and is non-empty
wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits exists and is non-empty
wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits exists and is non-empty
wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:32:19.616 +22:00:01.42
Second-epoch image center 05:32:18.221 +21:59:52.64
Angular distance between the image centers 0.0059 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:32:19.616 +22:00:01.42
Second-epoch image center 05:32:18.908 +22:00:21.48
Angular distance between the image centers 0.0062 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 05:32:18.221 +21:59:52.64
Second-epoch second image center 05:32:18.908 +22:00:21.48
Angular distance between the image centers 0.00844 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/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits &> /tmp/tmp.ZvUa2yCMMd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits &> /tmp/tmp.3sbUfY08eO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits &> /tmp/tmp.Hf7ZWIFBfj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits &> /tmp/tmp.hodpcMPjZi
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits and wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits and wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
Found non-empty wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits and wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
The reference image (wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits) and catalog (wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat) found
'wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat' -> 'wcsmag.cat'
Read 163644 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 74.1103 to 91.6919 deg, Dec +16.3196 to +27.3524 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 74.1103 to 91.6919 deg, Dec 16.3196 to 27.3524 deg
Loaded 12375 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): 7170 out of 10499 total matches.
Matched with Tycho-2 10499 out of 163644 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.769457
a=0.000000 b=1.000000 c=22.769457
From vast_summary.log: estimated ref. image limiting mag.: -7.29
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.48
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.48
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 77 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
2.0 pix Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
2.3 pix fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits
2.3 pix fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
Limiting magnitude estimates:
15.5 mag. Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
15.5 mag. Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
13.8 mag. fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits
13.7 mag. fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 13.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ZvUa2yCMMd (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits' -> 'wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WCS-calibrated image found: wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Checking if the catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WCS catalog name: wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=55, blended=21410, passed=163589
Got 163589 stars (including 141908 good ones) from the SExtractor catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
util/solve_plate_with_UCAC5 got 163589 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits -region wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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.3sbUfY08eO (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits' -> 'wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WCS-calibrated image found: wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
Checking if the catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WCS catalog name: wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=54, blended=21418, passed=163772
Got 163772 stars (including 142086 good ones) from the SExtractor catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat
util/solve_plate_with_UCAC5 got 163772 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
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 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 929 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits -region wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.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.Hf7ZWIFBfj (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_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.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_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits
Checking if the catalog wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits
WCS catalog name: wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=2820, passed=51134
Got 51134 stars (including 48241 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits.cat
util/solve_plate_with_UCAC5 got 51134 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.52"
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 921 stars left (next iteration limit 1013)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits -region wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.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.hodpcMPjZi (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_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.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_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
Checking if the catalog wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
WCS catalog name: wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=2427, passed=46859
Got 46859 stars (including 44378 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits.cat
util/solve_plate_with_UCAC5 got 46859 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.53"
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits -region wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.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_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Saving fully-calibrated image wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.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_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
Saving fully-calibrated image wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.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_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-45-04_20.00sec_-4.90C_LIGHT_0009.fits
Saving fully-calibrated image wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.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_2026-04-02_CI_Tau-04-Q2b1x1_214647_TTUQ2b1x1_30476_V84DhyRA/wcs_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010.fits
Preparing the HTML report for the field Tau-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out186195.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186217.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186219.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186229.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190716.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192497.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193629.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195259.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out188059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out188151.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190525.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192367.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192397.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 186194_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 186194_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:35:48.75 +25:04:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186195_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 186195_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:08:07.06 +20:53:36.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)
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Considering the candidate 186200_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 186200_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:49:42.14 +20:52:51.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186211_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 186211_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:44:21.12 +18:32:42.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186213_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 186213_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:46:26.61 +25:17:06.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186215_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 186215_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:42:04.64 +21:41:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186217_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 186217_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:57:18.74 +20:40:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 0.424 3423051212217763456 089.32797216677 +20.67861098634 12.9158 12.5601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.424#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 186218_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 186218_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:46:39.99 +23:50:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186219_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 186219_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:09:07.78 +21:52:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 3.086 3414991791984632320 077.28334043847 +21.88235750196 12.3952 11.6571 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.086#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 186220_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 186220_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:38:02.79 +22:27:13.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186223_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 186223_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:35:58.22 +24:15:07.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186225_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 186225_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:51:06.39 +22:35:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186229_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 186229_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:22:27.47 +19:14:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.32, MAG_FAINT_SEARCH_LIMIT=12.30)GAIADR2_OUTPUT=# 1.623 3401510022784985216 080.61473007727 +19.24117612515 11.5315 11.3261 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.623#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 186231_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 186231_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:38:22.89 +22:40:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 187248_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 187248_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:09:43.10 +23:02:03.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 188059_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
Preparing report for the candidate 188059_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
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Considering the candidate 188151_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
Preparing report for the candidate 188151_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
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Considering the candidate 188515_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 188515_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:41:56.07 +22:38:55.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 188683_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 188683_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:58:01.78 +25:55:16.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 189050_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 189050_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:30:07.90 +21:23:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 189847_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 189847_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:37:03.69 +20:44:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190035_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 190035_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:30:50.66 +22:27:24.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 190217_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 190217_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:45:44.92 +23:44:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190523_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 190523_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:48:36.02 +23:46:15.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190525_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
Preparing report for the candidate 190525_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
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Considering the candidate 190651_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 190651_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:43:00.27 +18:59:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190716_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 190716_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:49:21.67 +18:36:27.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 0.898 3398404868807802496 087.34009778014 +18.60780756381 12.5289 12.0474 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.898#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 190792_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 190792_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:41:08.58 +21:18:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190937_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 190937_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:45:36.96 +25:05:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191113_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 191113_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:32:09.86 +18:33:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191197_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 191197_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:45:54.24 +26:06:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191331_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 191331_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:37:00.55 +20:46:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191515_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 191515_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:45:50.20 +21:18:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191862_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 191862_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:47:13.73 +21:51:55.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191895_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 191895_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:31:40.03 +18:13:13.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191901_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 191901_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:48:06.77 +21:33:34.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192002_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 192002_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:51:30.85 +18:25:27.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192115_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 192115_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:42:11.78 +22:40:39.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 192216_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 192216_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:42:46.93 +21:22:23.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192273_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 192273_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:11:14.91 +23:03:10.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192367_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
Preparing report for the candidate 192367_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
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Considering the candidate 192380_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 192380_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:34:54.62 +19:28:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192397_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
Preparing report for the candidate 192397_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
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Considering the candidate 192435_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 192435_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:58:48.21 +25:47:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192497_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 192497_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:44:21.94 +21:11:09.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 2.992 3403072604903270272 086.09176538426 +21.18673695407 13.4715 12.9836 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.992#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192521_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 192521_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:33:38.32 +18:33:24.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 192679_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 192679_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:44:42.31 +23:00:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192724_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 192724_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:31:10.92 +20:10:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192864_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 192864_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:46:40.05 +20:11:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192969_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 192969_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:44:04.00 +24:38:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192981_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 192981_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:39:37.27 +18:52:55.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193196_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 193196_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:45:52.29 +21:18:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193202_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 193202_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:45:11.20 +18:40:43.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193218_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 193218_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:39:11.36 +19:48:10.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193315_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 193315_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:35:18.94 +21:12:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193339_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 193339_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:51:02.32 +20:08:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193439_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 193439_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:29:17.20 +18:20:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193440_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 193440_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:36:07.82 +19:32:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193506_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 193506_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:34:54.83 +22:33:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193629_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 193629_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:43:03.93 +23:33:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 3.149 3428373089014926976 085.76728468725 +23.56226367050 13.4861 12.9367 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.149#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193934_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 193934_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:35:28.98 +21:16:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193959_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 193959_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:20:11.60 +19:34:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193963_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 193963_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:30:36.35 +22:27:35.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 194033_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 194033_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:47:29.15 +18:44:55.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194205_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 194205_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:47:05.58 +23:11:12.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194299_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 194299_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:50:58.75 +22:40:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194338_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 194338_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:43:53.44 +21:56:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194372_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 194372_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:52:10.91 +22:50:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194427_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 194427_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:44:28.71 +22:45:57.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194442_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 194442_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:28:32.26 +22:45:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194768_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 194768_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:34:56.33 +20:14:27.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195259_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 195259_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:46:46.56 +21:31:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 1.249 3400179308775357696 086.69374518754 +21.52558672998 13.9480 13.4253 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.249#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195481_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 195481_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:39:27.33 +21:47:34.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 56342_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 56342_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:16:29.01 +20:02:20.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29777_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 29777_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:18:00.38 +18:21:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 89732_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 89732_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks
**** FOUND 05:08:17.01 +21:56:44.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18025_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010
The candidate 18025_fd_Tau-04-Q2b1x1_2026-04-02_21-46-00_20.00sec_-4.90C_LIGHT_0010 did not pass the final checks