This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC
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,2461139.7266,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.2266 13.51CV 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 J125.9153+55.7390,2461139.7266,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J125.9153+55.7390 20260409.2266 13.69CV 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
Gaia DR3 1081730020790023552,2461139.7266,13.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1081730020790023552 20260409.2266 13.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.2266* 08 45 14.27 +56 35 52.9 13.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EX UMa,2461139.7266,13.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
EX UMa 20260409.2266 13.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461139.7266,14.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.2266 14.49CV 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-Q2b1x1_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-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Last image: 2461139.72693691 09.04.2026 05:26:37.349 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
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: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 7562
Objects passed selection criteria: 7556
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 6945
Average stars matched: 6788.25 (97.743 %)
Memory usage VmPeak: 113980 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 00:31:33 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-Q2b1x1_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-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Last image: 2461139.72693691 09.04.2026 05:26:37.349 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 62
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.13
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: 20 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): 45500
Objects passed selection criteria: 45362
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 41995.5
Average stars matched: 40630.8 (96.7502 %)
Memory usage VmPeak: 148816 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 00:32:33 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
SExtractor catalog cache: saved Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat to cache
SExtractor catalog cache: saved Lyn-02-Q2b1x1_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-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.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: 2461139.72635672
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-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits exists and is non-empty
Saving wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits to local_wcs_cache/
'wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits' -> 'local_wcs_cache/wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits'
wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits exists and is non-empty
Saving wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits to local_wcs_cache/
'wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits' -> 'local_wcs_cache/wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits'
wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits exists and is non-empty
Saving wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits to local_wcs_cache/
'wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits' -> 'local_wcs_cache/wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits'
wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits exists and is non-empty
Saving wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits to local_wcs_cache/
'wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits' -> 'local_wcs_cache/wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits'
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# 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 08:28:46.819 +54:01:10.59
Angular distance between the image centers 0.0452 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:28:35.075 +53:59:05.09
Second-epoch image center 08:28:45.253 +54:00:48.03
Angular distance between the image centers 0.0379 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 08:28:46.819 +54:01:10.59
Second-epoch second image center 08:28:45.253 +54:00:48.03
Angular distance between the image centers 0.00735 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-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits &> /tmp/tmp.gOFOC3ztmu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_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-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits &> /tmp/tmp.P9hnyrkQPY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_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_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits &> /tmp/tmp.z2cSPSwF2d
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits &> /tmp/tmp.0UKdsoX6bW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-02-Q2b1x1_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-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q2b1x1_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-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
Found non-empty wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
The reference image (wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits) and catalog (wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat) found
'wcs_Lyn-02-Q2b1x1_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 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
2.1 pix Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
2.6 pix fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits
2.6 pix fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
Limiting magnitude estimates:
15.4 mag. Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
15.4 mag. Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
15.1 mag. fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits
15.1 mag. fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 12.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.gOFOC3ztmu (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits' -> 'wcs_Lyn-02-Q2b1x1_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-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS-calibrated image found: wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Checking if the catalog wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS catalog name: wcs_Lyn-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits -region wcs_Lyn-02-Q2b1x1_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-Q2b1x1_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.P9hnyrkQPY (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits' -> 'wcs_Lyn-02-Q2b1x1_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-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS-calibrated image found: wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Checking if the catalog wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS catalog name: wcs_Lyn-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits -region wcs_Lyn-02-Q2b1x1_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-Q2b1x1_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.z2cSPSwF2d (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits
WCS-calibrated image found: wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits
Checking if the catalog wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits.cat corresponding to the image wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits.cat corresponding to the image wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits
WCS catalog name: wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=543, passed=8981
Got 8981 stars (including 8433 good ones) from the SExtractor catalog wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits.cat
util/solve_plate_with_UCAC5 got 8981 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 8840 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 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(), 8838 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 8835 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 976 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits -region wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.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.0UKdsoX6bW (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
WCS-calibrated image found: wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
Checking if the catalog wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits.cat corresponding to the image wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits.cat corresponding to the image wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
WCS catalog name: wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=532, passed=8978
Got 8978 stars (including 8438 good ones) from the SExtractor catalog wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits.cat
util/solve_plate_with_UCAC5 got 8978 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 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(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 8832 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 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(), 8833 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 8833 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
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-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits -region wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.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-Q2b1x1_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-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits'
Saving fully-calibrated image wcs_Lyn-02-Q2b1x1_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-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits'
Saving fully-calibrated image wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits'
Saving fully-calibrated image wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits'
Preparing the HTML report for the field Lyn-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20533.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20382_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 20382_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:40:49.46 +50:08:13.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20533_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 20533_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 09:10:52.16 +56:15:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 1.663 1024417186918553088 137.71791169675 +56.26055411227 12.4913 11.9852 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.663#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Lyn-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
SExtractor catalog cache: saved Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat to cache
SExtractor catalog cache: saved Lyn-02-Q2b1x1_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-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Creating symlink local_wcs_cache/wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.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-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits exists and is non-empty
wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits exists and is non-empty
wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits exists and is non-empty
wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits exists and is non-empty
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# 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 08:28:46.819 +54:01:10.59
Angular distance between the image centers 0.0452 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:28:35.075 +53:59:05.09
Second-epoch image center 08:28:45.253 +54:00:48.03
Angular distance between the image centers 0.0379 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 08:28:46.819 +54:01:10.59
Second-epoch second image center 08:28:45.253 +54:00:48.03
Angular distance between the image centers 0.00735 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-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits &> /tmp/tmp.3C7ICBPHBo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_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-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits &> /tmp/tmp.suKBP2Xoud
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_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_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits &> /tmp/tmp.Jxyjxv9iGr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits &> /tmp/tmp.ZogMGNnCLq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-02-Q2b1x1_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-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q2b1x1_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-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
Found non-empty wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
The reference image (wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits) and catalog (wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat) found
'wcs_Lyn-02-Q2b1x1_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 22.045955
a=0.000000 b=1.000000 c=22.045955
From vast_summary.log: estimated ref. image limiting mag.: -7.13
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.92
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.92
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 51 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
2.0 pix Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
2.2 pix fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits
2.2 pix fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
Limiting magnitude estimates:
14.9 mag. Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
14.9 mag. Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
14.6 mag. fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits
14.6 mag. fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.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.3C7ICBPHBo (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits' -> 'wcs_Lyn-02-Q2b1x1_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-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS-calibrated image found: wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Checking if the catalog wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS catalog name: wcs_Lyn-02-Q2b1x1_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=14, blended=3457, passed=60976
Got 60976 stars (including 57414 good ones) from the SExtractor catalog wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
util/solve_plate_with_UCAC5 got 60976 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(), 9053 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(), 9089 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.39"
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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits -region wcs_Lyn-02-Q2b1x1_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-Q2b1x1_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.suKBP2Xoud (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits' -> 'wcs_Lyn-02-Q2b1x1_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-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS-calibrated image found: wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Checking if the catalog wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS catalog name: wcs_Lyn-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits -region wcs_Lyn-02-Q2b1x1_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-Q2b1x1_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.Jxyjxv9iGr (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits
WCS-calibrated image found: wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits
Checking if the catalog wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits.cat corresponding to the image wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits.cat corresponding to the image wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits
WCS catalog name: wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=2637, passed=50068
Got 50068 stars (including 47372 good ones) from the SExtractor catalog wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits.cat
util/solve_plate_with_UCAC5 got 50068 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 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(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 49337 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 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(), 49337 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 49337 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
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-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits -region wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.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.ZogMGNnCLq (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
WCS-calibrated image found: wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
Checking if the catalog wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits.cat corresponding to the image wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits.cat corresponding to the image wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
WCS catalog name: wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=2593, passed=49961
Got 49961 stars (including 47310 good ones) from the SExtractor catalog wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits.cat
util/solve_plate_with_UCAC5 got 49961 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 49218 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 49217 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 49217 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits -region wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.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-Q2b1x1_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_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Saving fully-calibrated image wcs_Lyn-02-Q2b1x1_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_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Saving fully-calibrated image wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-25-47_20.00sec_-5.00C_LIGHT_0185.fits
Saving fully-calibrated image wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lyn-02-Q2b1x1_002731_TTUQ2b1x1_3485_X3cpXlnC/wcs_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186.fits
Preparing the HTML report for the field Lyn-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out74347.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74350.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74353.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74355.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74359.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74360.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74362.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74365.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74369.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74382.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74780.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74921.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74958.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75198.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75244.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75271.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75278.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75319.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75362.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75401.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75405.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75435.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75487.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75512.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75529.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75542.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75547.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75562.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75563.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75589.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out75618.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out75074.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75174.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75220.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75269.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75557.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 18s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
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Considering the candidate 74347_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 74347_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:08:08.06 +50:40:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 0.448 935347158701667328 122.03346522228 +50.67501183698 15.1794 14.6655 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74350_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 74350_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:13:29.41 +56:59:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 2.683 1033505681314372864 123.37382508436 +56.99590864412 15.3384 14.6810 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.683#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74353_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 74353_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:14:26.18 +56:44:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 1.387 1033487401933558144 123.60926819892 +56.73915593968 14.6912 13.9876 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74355_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 74355_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:10:01.74 +52:41:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 1.275 935621211974588928 122.50736856826 +52.69098567592 15.2327 14.6871 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.275#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 74359_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 74359_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 09:03:35.21 +54:26:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 0.067 1023831353379286528 135.89672967846 +54.44518071254 14.7574 14.0533 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.067#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 74360_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 74360_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:21:17.58 +50:11:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 0.465 932140467398406144 125.32305228116 +50.19338643600 14.6531 14.1514 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 74362_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 74362_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:29:24.23 +56:24:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 0.788 1034015545471441408 127.35063945485 +56.40764829936 14.8372 14.3312 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.788#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 74365_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 74365_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:03:00.40 +49:35:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 2.133 934811318581120768 120.75084875120 +49.58823631029 14.9324 14.5071 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.133#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 74366_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 74366_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:01:24.60 +49:58:28.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74369_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 74369_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:06:43.98 +54:21:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.229 1032779385164100480 121.68383060495 +54.35173229252 14.6433 14.0411 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.229#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 74378_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 74378_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:33:53.13 +56:23:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74382_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 74382_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:10:58.06 +50:55:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 0.444 935189997257643904 122.74200322563 +50.92577714105 13.5039 12.9512 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.444#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 74527_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 74527_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:02:15.66 +51:17:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74605_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 74605_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:10:11.04 +55:47:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74621_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 74621_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:08:37.62 +51:32:04.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74628_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 74628_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:09:34.27 +55:10:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74638_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 74638_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:15:57.66 +50:46:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74780_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 74780_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:04:37.74 +53:56:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 1.316 1032746017562325632 121.15786710709 +53.94148537496 13.2053 12.6772 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.316#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 74880_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 74880_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:25:11.69 +54:30:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74921_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 74921_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:13:22.53 +52:32:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 0.604 1031634106364761088 123.34400309385 +52.54837077684 13.7179 13.2146 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.604#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 74951_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 74951_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:20:27.34 +51:18:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74958_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 74958_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:28:33.00 +56:48:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 0.809 1034106736217020544 127.13714181670 +56.81483465073 14.0084 13.4390 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.809#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75074_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
Preparing report for the candidate 75074_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
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Considering the candidate 75174_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
Preparing report for the candidate 75174_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
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Considering the candidate 75182_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 75182_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:25:51.86 +57:58:58.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75198_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 75198_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:08:32.58 +53:57:53.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 0.074 1032569859479439360 122.13576680084 +53.96489850465 14.4348 13.9788 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.074#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75207_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 75207_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:03:49.72 +55:19:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 1.706 1032974617197621504 120.95657077186 +55.32266450127 14.6297 13.8630 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.706#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75220_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
Preparing report for the candidate 75220_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
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Considering the candidate 75244_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 75244_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:05:50.63 +50:17:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 0.691 934950647320632832 121.46095968666 +50.29125243728 14.4095 13.9692 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.691#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75269_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
Preparing report for the candidate 75269_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
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Considering the candidate 75271_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 75271_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:16:42.33 +54:03:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 1.547 1031868199262047872 124.17710217252 +54.05096509709 14.6020 14.1150 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.547#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75278_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 75278_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:01:09.55 +53:16:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 1.522 936632895815368960 120.28935657617 +53.27480541157 14.7999 14.2268 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.522#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75280_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 75280_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:11:11.40 +50:06:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75302_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 75302_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:30:19.24 +54:28:48.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75319_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 75319_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:01:37.74 +55:27:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 0.548 1081025062038385792 120.40748389134 +55.46656419159 14.5680 14.1201 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.548#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75362_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 75362_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:04:24.08 +52:57:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 0.786 936425882687047424 121.10049459412 +52.95814008664 14.6486 14.1083 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.786#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75401_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 75401_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:11:07.48 +55:06:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 0.237 1033106249355025280 122.78108299683 +55.10351028833 14.9317 14.3719 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.237#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75405_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 75405_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:07:17.36 +53:32:17.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 0.285 1032534228430804608 121.82244330368 +53.53829467011 15.0597 14.7259 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.285#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75435_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 75435_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:06:15.23 +51:02:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 1.914 935416565373173248 121.56365940095 +51.04534987822 14.9966 14.4665 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.914#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75487_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 75487_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:14:12.45 +57:27:30.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 1.857 1035069801027864448 123.55092755168 +57.45863489331 14.8875 14.3343 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.857#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75512_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 75512_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:23:56.82 +57:26:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 0.430 1034902473398176640 125.98673014167 +57.44826993436 14.7988 14.1142 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.430#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75529_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 75529_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:02:41.80 +57:27:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 1.098 1081849283441862784 120.67363495105 +57.45775485426 14.9889 14.3732 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.098#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75542_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 75542_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:23:52.72 +54:54:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 1.729 1032346761698253056 125.97048893872 +54.90269306045 15.1280 14.5723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.729#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75547_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 75547_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 07:59:49.86 +52:37:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.59, MAG_FAINT_SEARCH_LIMIT=15.57)GAIADR2_OUTPUT=# 0.346 936496629388467456 119.95760780981 +52.61962556430 15.1405 14.6129 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.346#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75557_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
Preparing report for the candidate 75557_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
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Considering the candidate 75562_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 75562_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:48:29.14 +49:50:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 3.565 1015238085893633536 132.12045627842 +49.84932845359 14.9668 14.3639 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.565#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75563_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 75563_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:07:40.40 +49:38:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 0.924 934727412100050944 121.91858136418 +49.64957753700 14.9021 14.2324 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.924#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75589_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 75589_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:11:13.97 +50:02:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 0.185 934707792689352448 122.80826829791 +50.03679918807 15.0602 14.5302 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.185#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75591_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 75591_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:05:03.84 +49:48:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 0.955 934840936675575808 121.26588203661 +49.80361523604 15.0748 14.5371 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.955#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75618_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 75618_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks
**** FOUND 08:30:37.58 +51:06:19.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)
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Considering the candidate 48804_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186
The candidate 48804_fd_Lyn-02-Q2b1x1_2026-04-09_00-26-37_20.00sec_-4.90C_LIGHT_0186 did not pass the final checks