This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.7199,14.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.2199 14.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J116.8685+52.9527,2461146.7199,13.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J116.8685+52.9527 20260416.2199 13.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.7199,14.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.2199 14.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J117.3403+57.5393,2461146.7199,14.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J117.3403+57.5393 20260416.2199 14.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.7199,14.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.2199 14.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.7199,14.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.2199 14.30CV 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: 2461058.81301528 18.01.2026 07:30:34.520 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
First image: 2461058.81301528 18.01.2026 07:30:34.520 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Last image: 2461146.72028744 16.04.2026 05:17:02.835 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.42
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: 3 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): 10323
Objects passed selection criteria: 10313
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 9781.25
Average stars matched: 9626.75 (98.4204 %)
Memory usage VmPeak: 115636 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 16 00:21:06 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: 2461058.81301528 18.01.2026 07:30:34.520 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
First image: 2461058.81301528 18.01.2026 07:30:34.520 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Last image: 2461146.72028744 16.04.2026 05:17:02.835 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 74
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.20
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: 19 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): 59574
Objects passed selection criteria: 59414
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 57380.2
Average stars matched: 55717 (97.1014 %)
Memory usage VmPeak: 160560 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 16 00:22:03 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/TTUQ1b1x1/TTUQ1_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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
SExtractor catalog cache: saved Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat to cache
SExtractor catalog cache: saved Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.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/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461146.71950274
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits exists and is non-empty
Saving wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits to local_wcs_cache/
'wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits' -> 'local_wcs_cache/wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits'
wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits exists and is non-empty
Saving wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits to local_wcs_cache/
'wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits' -> 'local_wcs_cache/wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits'
wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits exists and is non-empty
Saving wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits to local_wcs_cache/
'wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits' -> 'local_wcs_cache/wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits'
wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits exists and is non-empty
Saving wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits to local_wcs_cache/
'wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits' -> 'local_wcs_cache/wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits (1st reference image)
verification OK: wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Image size: 927.4'x629.8' 15.5(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.92"/pix along the Y axis
Image center: 08:28:35.075 +53:59:05.09 J2000 4789.000 3195.000
###################################
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
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# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits (1st new image)
verification OK: wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits
Image size: 941.5'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:28:26.123 +53:57:41.32 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:28:35.075 +53:59:05.09
Second-epoch image center 08:28:26.123 +53:57:41.32
Angular distance between the image centers 0.0320 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits (2nd new image)
verification OK: wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
Image size: 941.5'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:28:29.011 +53:57:42.03 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:28:35.075 +53:59:05.09
Second-epoch image center 08:28:29.011 +53:57:42.03
Angular distance between the image centers 0.0274 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 08:28:26.123 +53:57:41.32
Second-epoch second image center 08:28:29.011 +53:57:42.03
Angular distance between the image centers 0.00708 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/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits &> /tmp/tmp.p4UIGfICQm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits &> /tmp/tmp.DSZriCGCdc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits &> /tmp/tmp.MUu8EXRgR5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits &> /tmp/tmp.s7BAIZAsDe
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.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_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.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_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
Found non-empty wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
The reference image (wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits) and catalog (wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat) found
'wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat' -> 'wcsmag.cat'
Read 10732 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 113.1029 to 142.4921 deg, Dec +47.7241 to +59.2635 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 113.1029 to 142.4921 deg, Dec 47.7241 to 59.2635 deg
Loaded 7241 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): 20 out of 20 total matches.
Matched with Tycho-2 20 out of 10732 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.854505
a=0.000000 b=1.000000 c=22.854505
From vast_summary.log: estimated ref. image limiting mag.: -7.42
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.43
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.43
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
2.1 pix Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
2.1 pix fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits
2.1 pix fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
Limiting magnitude estimates:
15.4 mag. Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
15.4 mag. Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
15.2 mag. fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits
15.2 mag. fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 12.2 (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.p4UIGfICQm (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits' -> 'wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS-calibrated image found: wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Checking if the catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS catalog name: wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=751, passed=10732
Got 10732 stars (including 9968 good ones) from the SExtractor catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
util/solve_plate_with_UCAC5 got 10732 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.4'
Seting catalog search parameters based on the expected field of view 927.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012881 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010304 (37.1 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 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 178 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 147 matched stars entering correct_measured_positions(), 124 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 10.17"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 141 matched stars entering correct_measured_positions(), 1637 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.63"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 223 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 205 matched stars entering correct_measured_positions(), 1671 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.34"
Accuracy estimation diagnostic: 202 matched stars entering correct_measured_positions(), 2144 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.08"
Excluding outliers - 202 stars left (next iteration limit 155)
The image catalog is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits -region wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.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.DSZriCGCdc (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits' -> 'wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS-calibrated image found: wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Checking if the catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS catalog name: wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=785, passed=10668
Got 10668 stars (including 9872 good ones) from the SExtractor catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat
util/solve_plate_with_UCAC5 got 10668 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.5'
Seting catalog search parameters based on the expected field of view 927.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012882 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010306 (37.1 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 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 172 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 142 matched stars entering correct_measured_positions(), 117 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 11.19"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 137 matched stars entering correct_measured_positions(), 1584 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.80"
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 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 219 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 199 matched stars entering correct_measured_positions(), 1618 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.56"
Accuracy estimation diagnostic: 198 matched stars entering correct_measured_positions(), 2106 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.06"
Excluding outliers - 198 stars left (next iteration limit 150)
The image catalog is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits -region wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.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.MUu8EXRgR5 (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_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.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_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits
WCS-calibrated image found: wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits
Checking if the catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits
WCS catalog name: wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=635, passed=8983
Got 8983 stars (including 8335 good ones) from the SExtractor catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits.cat
util/solve_plate_with_UCAC5 got 8983 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 8862 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
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 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 8862 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 8862 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits -region wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.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.s7BAIZAsDe (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_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.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_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
WCS-calibrated image found: wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
Checking if the catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
WCS catalog name: wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=632, passed=8990
Got 8990 stars (including 8352 good ones) from the SExtractor catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits.cat
util/solve_plate_with_UCAC5 got 8990 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 8859 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
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 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 8859 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 8859 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits -region wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.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_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits'
Saving fully-calibrated image wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits'
Saving fully-calibrated image wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits'
Saving fully-calibrated image wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits'
Preparing the HTML report for the field Lyn-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20520.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20522.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20506_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 20506_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:40:49.50 +50:08:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20518_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 20518_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:28:18.78 +55:46:33.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20520_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 20520_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 09:15:11.13 +54:04:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 0.668 1022872265706057856 138.79667739493 +54.08269324303 12.3439 11.7737 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.668#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20522_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 20522_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:22:24.55 +56:27:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 1.683 1034740806533360384 125.60273977697 +56.45302009656 12.3628 11.8277 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.683#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02150_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 02150_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:55:51.05 +57:11:51.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Lyn-02-Q1b1x1 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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
SExtractor catalog cache: saved Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat to cache
SExtractor catalog cache: saved Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Creating symlink local_wcs_cache/wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.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_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits exists and is non-empty
wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits exists and is non-empty
wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits exists and is non-empty
wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits (1st reference image)
verification OK: wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Image size: 927.4'x629.8' 15.5(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.92"/pix along the Y axis
Image center: 08:28:35.075 +53:59:05.09 J2000 4789.000 3195.000
###################################
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits (1st new image)
verification OK: wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits
Image size: 941.5'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:28:26.123 +53:57:41.32 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:28:35.075 +53:59:05.09
Second-epoch image center 08:28:26.123 +53:57:41.32
Angular distance between the image centers 0.0320 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits (2nd new image)
verification OK: wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
Image size: 941.5'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:28:29.011 +53:57:42.03 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:28:35.075 +53:59:05.09
Second-epoch image center 08:28:29.011 +53:57:42.03
Angular distance between the image centers 0.0274 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 08:28:26.123 +53:57:41.32
Second-epoch second image center 08:28:29.011 +53:57:42.03
Angular distance between the image centers 0.00708 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/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits &> /tmp/tmp.ABVrsAPu0p
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits &> /tmp/tmp.nv4EmpSeno
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits &> /tmp/tmp.fR4zPtOBhL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits &> /tmp/tmp.ShtiyE3fuw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.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_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.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_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
Found non-empty wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
The reference image (wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits) and catalog (wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat) found
'wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat' -> 'wcsmag.cat'
Read 60990 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 113.0237 to 142.6172 deg, Dec +47.6792 to +59.2703 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 113.0237 to 142.6172 deg, Dec 47.6792 to 59.2703 deg
Loaded 7317 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): 20 out of 25 total matches.
Matched with Tycho-2 25 out of 60990 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.056610
a=0.000000 b=1.000000 c=22.056610
From vast_summary.log: estimated ref. image limiting mag.: -7.20
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.86
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.86
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 68 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
2.0 pix Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
2.0 pix fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits
2.0 pix fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
Limiting magnitude estimates:
14.9 mag. Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
14.9 mag. Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
14.6 mag. fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits
14.6 mag. fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 14.0 (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.ABVrsAPu0p (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits' -> 'wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS-calibrated image found: wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Checking if the catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS catalog name: wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=3457, passed=60971
Got 60971 stars (including 57409 good ones) from the SExtractor catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
util/solve_plate_with_UCAC5 got 60971 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.4'
Seting catalog search parameters based on the expected field of view 927.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012881 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010304 (37.1 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 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 172 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 142 matched stars entering correct_measured_positions(), 118 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.89"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 135 matched stars entering correct_measured_positions(), 9052 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.46"
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 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 218 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 192 matched stars entering correct_measured_positions(), 9088 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.40"
Accuracy estimation diagnostic: 189 matched stars entering correct_measured_positions(), 12156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.55"
Excluding outliers - 189 stars left (next iteration limit 148)
The image catalog is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits -region wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.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.nv4EmpSeno (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits' -> 'wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS-calibrated image found: wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Checking if the catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS catalog name: wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=3501, passed=61060
Got 61060 stars (including 57445 good ones) from the SExtractor catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat
util/solve_plate_with_UCAC5 got 61060 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.5'
Seting catalog search parameters based on the expected field of view 927.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012882 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010306 (37.1 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 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 172 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 140 matched stars entering correct_measured_positions(), 117 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 10.18"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 133 matched stars entering correct_measured_positions(), 8718 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.40"
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 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 219 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 189 matched stars entering correct_measured_positions(), 8757 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.37"
Accuracy estimation diagnostic: 188 matched stars entering correct_measured_positions(), 12273 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.11"
Excluding outliers - 188 stars left (next iteration limit 146)
The image catalog is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits -region wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.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.fR4zPtOBhL (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_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.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_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits
WCS-calibrated image found: wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits
Checking if the catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits
WCS catalog name: wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=2868, passed=54799
Got 54799 stars (including 51824 good ones) from the SExtractor catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits.cat
util/solve_plate_with_UCAC5 got 54799 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 54334 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 54334 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 54333 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits -region wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.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.ShtiyE3fuw (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_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.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_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
WCS-calibrated image found: wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
Checking if the catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
WCS catalog name: wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=2812, passed=54322
Got 54322 stars (including 51415 good ones) from the SExtractor catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits.cat
util/solve_plate_with_UCAC5 got 54322 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 53839 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 53839 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 53839 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits -region wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.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_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.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_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Saving fully-calibrated image wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.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_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Saving fully-calibrated image wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.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_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-15-55_20.00sec_-5.00C_LIGHTs_0146.fits
Saving fully-calibrated image wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.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_2026-04-16_CI_Lyn-02-Q1b1x1_001801_TTUQ1b1x1_16079_FPqdiBil/wcs_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147.fits
Preparing the HTML report for the field Lyn-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out75396.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75401.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75414.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75627.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75639.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75692.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75719.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75740.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75742.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75764.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75771.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75777.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75787.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75791.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75793.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75795.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75806.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75825.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75827.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75829.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75831.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75835.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75845.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75855.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75874.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75876.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75886.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75888.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75894.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75898.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75946.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out76001.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out76019.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out75409.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75796.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75805.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75816.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75868.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75934.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 20s
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 75396_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75396_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:48:53.69 +55:19:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 1.351 985122221889933184 117.22389860226 +55.32241851116 14.9467 14.4340 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.351#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75401_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75401_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:56:24.72 +55:11:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 0.869 1080961874479346048 119.10290768746 +55.18620884004 14.4265 13.6645 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.869#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75409_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
Preparing report for the candidate 75409_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
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Considering the candidate 75414_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75414_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:21:17.61 +50:11:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 1.682 932140467398406144 125.32305228116 +50.19338643600 14.6531 14.1514 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.682#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75417_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75417_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:39:34.54 +54:23:42.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)
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Considering the candidate 75430_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75430_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:33:53.15 +56:23:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75431_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75431_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:51:44.15 +49:23:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75434_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75434_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:11:25.40 +56:03:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75435_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75435_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:19:58.24 +55:53:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75448_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75448_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:14:03.32 +49:24:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75462_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75462_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:10:11.04 +55:47:08.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75470_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75470_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:09:34.30 +55:10:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75471_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75471_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:08:37.64 +51:32:04.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75481_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75481_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:45:02.97 +55:43:53.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75485_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75485_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:08:33.07 +49:01:48.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75552_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75552_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:35:35.00 +56:54:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75561_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75561_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:48:59.34 +56:45:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75566_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75566_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:17:19.08 +58:59:27.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75575_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75575_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:28:33.04 +56:48:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75596_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75596_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:59:02.66 +58:53:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75627_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75627_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:47:15.99 +55:12:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 1.459 1030813355295281408 131.81598567410 +55.20435141101 14.1198 13.2732 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.459#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75635_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75635_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:48:49.14 +55:26:42.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75639_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75639_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:56:57.35 +53:57:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 1.603 984754843271176576 119.23833700226 +53.95255992597 14.2610 13.2897 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.603#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75641_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75641_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:46:56.76 +55:21:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75692_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75692_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:44:09.89 +51:39:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 2.758 982782392426138624 116.04243793501 +51.66445535678 14.5633 14.1242 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.758#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75719_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75719_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:01:09.53 +53:16:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 2.612 936632895815368960 120.28935657617 +53.27480541157 14.7999 14.2268 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.612#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75723_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75723_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:46:10.76 +57:28:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 0.405 1082412538340547328 116.54471225871 +57.48251927682 14.6188 14.0282 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.405#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75740_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75740_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:33:04.96 +57:51:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 2.269 1034632096618335488 128.27005977232 +57.85181911476 14.7633 14.1297 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.269#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75742_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75742_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:57:35.31 +58:56:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 1.479 1082749474227361408 119.39762906973 +58.94182066297 14.7832 14.2360 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.479#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75764_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75764_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:45:33.22 +55:27:49.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 1.510 985885763996062848 116.38769838493 +55.46359335294 14.7382 14.1068 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.510#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75771_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75771_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:36:40.40 +53:24:13.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 0.576 983749447262952192 114.16831606216 +53.40361812732 15.0289 14.4936 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.576#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75777_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75777_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:38:50.16 +54:59:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 2.867 985629096750151680 114.70770448330 +54.98799174551 14.8910 14.2004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75783_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75783_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:40:55.36 +56:29:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75787_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75787_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:58:09.02 +58:30:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 2.290 1082704944006598016 119.53835693647 +58.51039767087 14.8051 14.2757 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.290#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75791_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75791_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:21:07.38 +58:47:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 0.610 1035579325884059264 125.28055346496 +58.79261453698 14.8655 14.0702 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.610#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75793_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75793_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:45:08.47 +56:29:13.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 2.132 1082078119299586688 116.28635413263 +56.48719180381 15.0746 14.5226 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.132#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75795_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75795_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:36:12.11 +56:10:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 1.430 986131676643014016 114.05046182476 +56.18138065214 14.8649 14.3817 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.430#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75796_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
Preparing report for the candidate 75796_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
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Considering the candidate 75798_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75798_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:46:08.50 +52:10:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 0.521 984320437394658560 116.53521158310 +52.18037702767 14.8445 14.3573 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.521#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75805_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
Preparing report for the candidate 75805_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
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Considering the candidate 75806_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75806_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:05:48.22 +59:07:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 0.119 1083464122425563264 121.45086052152 +59.12081703970 15.1011 14.5272 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.119#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75814_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75814_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:23:52.89 +54:54:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75816_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
Preparing report for the candidate 75816_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
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Considering the candidate 75825_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75825_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:35:36.21 +58:52:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 2.528 1085598068337432448 113.89974233459 +58.87258467689 14.7611 14.2303 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.528#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75827_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75827_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:13:15.00 +49:36:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 2.534 931681180775785472 123.31255139312 +49.59960255332 14.7911 13.8513 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.534#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75829_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75829_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:51:05.32 +58:00:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 1.557 1082630005417043968 117.77195456720 +58.00838983000 14.9473 14.4421 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.557#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75831_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75831_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:37:55.38 +56:11:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 1.445 986123121068140800 114.48057486195 +56.19005496497 14.9920 14.5484 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.445#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75835_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75835_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:41:08.30 +57:03:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 1.296 1082341795931695872 115.28461651336 +57.06266827395 14.8605 14.2917 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.296#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75845_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75845_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:41:56.61 +55:35:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 1.448 985858757241565952 115.48524159268 +55.58367758141 15.1135 14.5997 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75847_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75847_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:31:14.77 +58:56:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75849_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75849_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:24:17.65 +57:48:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75853_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75853_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:09:30.09 +58:48:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75855_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75855_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:53:08.44 +51:03:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 0.937 935978106576807552 118.28557027689 +51.05449694504 15.0836 14.6121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.937#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75868_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
Preparing report for the candidate 75868_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
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Considering the candidate 75874_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75874_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:46:23.90 +57:12:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 1.810 1082127081926609792 116.59996334694 +57.21140235154 14.9501 14.4697 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.810#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75876_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75876_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 09:21:46.24 +55:25:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 1.434 1023429928555582208 140.44264899921 +55.43190722590 15.0772 14.5644 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.434#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75886_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75886_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:44:02.46 +55:34:52.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 2.361 985937887719120896 116.01094267681 +55.58080708437 14.9898 13.8740 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.361#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75888_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75888_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:55:01.52 +49:08:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 0.658 934048394950449408 118.75639139879 +49.14073777594 15.1061 14.6419 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.658#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75894_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75894_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:02:41.75 +57:27:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 1.609 1081849283441862784 120.67363495105 +57.45775485426 14.9889 14.3732 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.609#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75898_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75898_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:50:41.78 +58:01:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.51, MAG_FAINT_SEARCH_LIMIT=15.49)GAIADR2_OUTPUT=# 0.790 1082629490020972672 117.67408604329 +58.01855838231 15.1079 14.5550 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.790#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75934_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
Preparing report for the candidate 75934_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
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Considering the candidate 75946_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75946_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:51:46.11 +53:09:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 1.106 984293636798313856 117.94186337206 +53.15118078715 15.1280 14.4157 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.106#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75947_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 75947_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:08:43.09 +55:33:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76001_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 76001_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:03:22.24 +49:38:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 0.547 934813139647250688 120.84250046189 +49.64371831384 14.8289 13.9600 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.547#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 76019_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 76019_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:59:56.43 +50:22:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 2.612 935676496793821440 119.98511653927 +50.37811440766 15.1489 14.6964 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.612#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 48804_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 48804_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 08:40:49.51 +50:08:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11108_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 11108_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks
**** FOUND 07:55:51.07 +57:11:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29752_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147
The candidate 29752_fd_Lyn-02-Q1b1x1_2026-04-16_00-17-02_20.00sec_-4.90C_LIGHTs_0147 did not pass the final checks