This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP
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
Gaia DR3 989251059850952576,2461140.8531,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 989251059850952576 20260410.3531 12.97CV 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 J123.6714+57.9648,2461140.8531,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J123.6714+57.9648 20260410.3531 13.19CV 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
Mean magnitude and position on the discovery images:
2026 04 10.3531 2461140.8531 13.24 07:58:18.96 +54:01:54.1
164.10055 31.29386 galactic Lyn Second-epoch detections are separated by 5.2" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 984776769079599744 | 07:58:15.08 +54:02:15.7 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: F9 (LAMOST DR5) J-Ks=0.250+/-0.040 (F)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
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
Large-amplitude variable Gaia DR2 984776769079599744,2461140.8531,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 984776769079599744 20260410.3531 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J125.9153+55.7390,2461140.8531,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J125.9153+55.7390 20260410.3531 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.81301528 18.01.2026 07:30:34.520 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
First image: 2461058.81301528 18.01.2026 07:30:34.520 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Last image: 2461140.85352453 10.04.2026 08:28:54.519 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
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: 5 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): 10122
Objects passed selection criteria: 10096
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 8603.25
Average stars matched: 8467 (98.4163 %)
Memory usage VmPeak: 115644 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 10 03:38:40 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.81301528 18.01.2026 07:30:34.520 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
First image: 2461058.81301528 18.01.2026 07:30:34.520 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Last image: 2461140.85352453 10.04.2026 08:28:54.519 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 72
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.20
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 16 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): 57192
Objects passed selection criteria: 57063
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 52227.2
Average stars matched: 50928.2 (97.5128 %)
Memory usage VmPeak: 157020 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 10 03:46:53 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
SExtractor catalog cache: saved Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat to cache
SExtractor catalog cache: saved Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461140.85274347
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits exists and is non-empty
Saving wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits to local_wcs_cache/
'wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits' -> 'local_wcs_cache/wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits'
wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits exists and is non-empty
Saving wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits to local_wcs_cache/
'wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits' -> 'local_wcs_cache/wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits'
wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits exists and is non-empty
Saving wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits to local_wcs_cache/
'wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits' -> 'local_wcs_cache/wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits'
wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits exists and is non-empty
Saving wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits to local_wcs_cache/
'wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits' -> 'local_wcs_cache/wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.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 08:28:44.486 +53:59:41.58
Angular distance between the image centers 0.0252 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 08:28:48.361 +54:00:09.56
Angular distance between the image centers 0.0371 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 08:28:44.486 +53:59:41.58
Second-epoch second image center 08:28:48.361 +54:00:09.56
Angular distance between the image centers 0.01227 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits &> /tmp/tmp.2sRDfFzaw3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits &> /tmp/tmp.qzpKUYfrG0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits &> /tmp/tmp.v2U39e1oE4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits &> /tmp/tmp.vl4Wvo31ak
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
Found non-empty wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
The reference image (wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits) and catalog (wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat) found
'wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat' -> 'wcsmag.cat'
Read 10732 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 113.1029 to 142.4921 deg, Dec +47.7241 to +59.2635 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 113.1029 to 142.4921 deg, Dec 47.7241 to 59.2635 deg
Loaded 7241 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 20 out of 20 total matches.
Matched with Tycho-2 20 out of 10732 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.854505
a=0.000000 b=1.000000 c=22.854505
From vast_summary.log: estimated ref. image limiting mag.: -7.42
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.43
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.43
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
2.1 pix Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
2.1 pix fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits
2.1 pix fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
Limiting magnitude estimates:
15.4 mag. Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
15.4 mag. Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
14.8 mag. fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits
14.8 mag. fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 11.8 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.2sRDfFzaw3 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits' -> 'wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS-calibrated image found: wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Checking if the catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS catalog name: wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=751, passed=10732
Got 10732 stars (including 9968 good ones) from the SExtractor catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
util/solve_plate_with_UCAC5 got 10732 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.4'
Seting catalog search parameters based on the expected field of view 927.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012881 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010304 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 178 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 147 matched stars entering correct_measured_positions(), 124 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 10.17"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 141 matched stars entering correct_measured_positions(), 1637 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.63"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 223 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 205 matched stars entering correct_measured_positions(), 1671 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.34"
Accuracy estimation diagnostic: 202 matched stars entering correct_measured_positions(), 2144 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.08"
Excluding outliers - 202 stars left (next iteration limit 155)
The image catalog is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits -region wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.qzpKUYfrG0 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits' -> 'wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS-calibrated image found: wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Checking if the catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS catalog name: wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=785, passed=10668
Got 10668 stars (including 9872 good ones) from the SExtractor catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat
util/solve_plate_with_UCAC5 got 10668 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.5'
Seting catalog search parameters based on the expected field of view 927.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012882 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010306 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 172 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 142 matched stars entering correct_measured_positions(), 117 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 11.19"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 137 matched stars entering correct_measured_positions(), 1584 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.80"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 219 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 199 matched stars entering correct_measured_positions(), 1618 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.56"
Accuracy estimation diagnostic: 198 matched stars entering correct_measured_positions(), 2106 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.06"
Excluding outliers - 198 stars left (next iteration limit 150)
The image catalog is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits -region wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.v2U39e1oE4 (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_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.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_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits
WCS-calibrated image found: wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits
Checking if the catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits
WCS catalog name: wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=414, passed=6626
Got 6626 stars (including 6205 good ones) from the SExtractor catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits.cat
util/solve_plate_with_UCAC5 got 6626 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 924.9'
Seting catalog search parameters based on the expected field of view 924.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012846 (46.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010277 (37.0 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 47.8 to 59.4)
Done reading UCAC5 zone files...
Matched 605 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 594 matched stars entering correct_measured_positions(), 577 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.71"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 594 matched stars entering correct_measured_positions(), 3966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.73"
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 47.8 to 59.4)
Done reading UCAC5 zone files...
Matched 636 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 630 matched stars entering correct_measured_positions(), 3974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.46"
Accuracy estimation diagnostic: 628 matched stars entering correct_measured_positions(), 4125 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.25"
Excluding outliers - 628 stars left (next iteration limit 653)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits -region wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.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.vl4Wvo31ak (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_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.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_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
WCS-calibrated image found: wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
Checking if the catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
WCS catalog name: wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=403, passed=6590
Got 6590 stars (including 6177 good ones) from the SExtractor catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits.cat
util/solve_plate_with_UCAC5 got 6590 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010467 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.4)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 6495 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 59.4)
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(), 6495 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 6495 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits -region wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits'
Saving fully-calibrated image wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits'
Saving fully-calibrated image wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits'
Saving fully-calibrated image wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits'
Preparing the HTML report for the field Lyn-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20506_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 20506_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
Rejecting candidate due to large distance (93.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02150_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 02150_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 07:55:51.11 +57:11:51.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 0s
Prepared the HTML report for the field Lyn-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
SExtractor catalog cache: saved Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat to cache
SExtractor catalog cache: saved Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Creating symlink local_wcs_cache/wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits exists and is non-empty
wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits exists and is non-empty
wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits exists and is non-empty
wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.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 08:28:44.486 +53:59:41.58
Angular distance between the image centers 0.0252 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 08:28:48.361 +54:00:09.56
Angular distance between the image centers 0.0371 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 08:28:44.486 +53:59:41.58
Second-epoch second image center 08:28:48.361 +54:00:09.56
Angular distance between the image centers 0.01227 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits &> /tmp/tmp.HeOVBQkHsH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits &> /tmp/tmp.sszl8tOxTG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits &> /tmp/tmp.fhwdHP4E7q
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits &> /tmp/tmp.TOwCPuCwYx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
Found non-empty wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
The reference image (wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits) and catalog (wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat) found
'wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat' -> 'wcsmag.cat'
Read 60990 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 113.0237 to 142.6172 deg, Dec +47.6792 to +59.2703 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 113.0237 to 142.6172 deg, Dec 47.6792 to 59.2703 deg
Loaded 7317 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 20 out of 25 total matches.
Matched with Tycho-2 25 out of 60990 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.056610
a=0.000000 b=1.000000 c=22.056610
From vast_summary.log: estimated ref. image limiting mag.: -7.20
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.86
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.86
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 52 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
2.0 pix Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
1.9 pix fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits
1.9 pix fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
Limiting magnitude estimates:
14.9 mag. Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
14.9 mag. Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
14.3 mag. fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits
14.3 mag. fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 13.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.HeOVBQkHsH (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits' -> 'wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS-calibrated image found: wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Checking if the catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS catalog name: wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=3457, passed=60971
Got 60971 stars (including 57409 good ones) from the SExtractor catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
util/solve_plate_with_UCAC5 got 60971 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.4'
Seting catalog search parameters based on the expected field of view 927.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012881 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010304 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 172 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 142 matched stars entering correct_measured_positions(), 118 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.89"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 135 matched stars entering correct_measured_positions(), 9052 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 218 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 192 matched stars entering correct_measured_positions(), 9088 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.40"
Accuracy estimation diagnostic: 189 matched stars entering correct_measured_positions(), 12156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.55"
Excluding outliers - 189 stars left (next iteration limit 148)
The image catalog is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits -region wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.sszl8tOxTG (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits' -> 'wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS-calibrated image found: wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Checking if the catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS catalog name: wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=3501, passed=61060
Got 61060 stars (including 57445 good ones) from the SExtractor catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat
util/solve_plate_with_UCAC5 got 61060 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.5'
Seting catalog search parameters based on the expected field of view 927.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012882 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010306 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 172 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 140 matched stars entering correct_measured_positions(), 117 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 10.18"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 133 matched stars entering correct_measured_positions(), 8718 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 219 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 189 matched stars entering correct_measured_positions(), 8757 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.37"
Accuracy estimation diagnostic: 188 matched stars entering correct_measured_positions(), 12273 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.11"
Excluding outliers - 188 stars left (next iteration limit 146)
The image catalog is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits -region wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.fhwdHP4E7q (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_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.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_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits
WCS-calibrated image found: wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits
Checking if the catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits
WCS catalog name: wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1754, passed=44186
Got 44186 stars (including 42354 good ones) from the SExtractor catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits.cat
util/solve_plate_with_UCAC5 got 44186 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 924.9'
Seting catalog search parameters based on the expected field of view 924.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012846 (46.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010277 (37.0 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 59.4)
Done reading UCAC5 zone files...
Matched 603 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 593 matched stars entering correct_measured_positions(), 577 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.63"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 593 matched stars entering correct_measured_positions(), 28161 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.61"
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 59.4)
Done reading UCAC5 zone files...
Matched 635 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 627 matched stars entering correct_measured_positions(), 28168 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.59"
Accuracy estimation diagnostic: 626 matched stars entering correct_measured_positions(), 29329 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.29"
Excluding outliers - 626 stars left (next iteration limit 652)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits -region wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.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.TOwCPuCwYx (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_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.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_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
WCS-calibrated image found: wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
Checking if the catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
WCS catalog name: wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=1704, passed=44075
Got 44075 stars (including 42288 good ones) from the SExtractor catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits.cat
util/solve_plate_with_UCAC5 got 44075 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010467 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.4)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 43561 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 59.4)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 43559 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 43559 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits -region wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Saving fully-calibrated image wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Saving fully-calibrated image wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.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_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-27-47_20.00sec_-4.90C_LIGHTs_0200.fits
Saving fully-calibrated image wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.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_2026-04-10_CI_Lyn-02-Q1b1x1_032950_TTUQ1b1x1_8136_3n70prNP/wcs_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201.fits
Preparing the HTML report for the field Lyn-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out38213.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75388.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75394.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75398.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75408.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75411.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75450.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75486.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75502.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75522.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75553.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75567.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75573.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75578.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75599.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75606.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75673.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75676.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75679.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75703.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75735.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75740.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75756.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75765.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75770.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75793.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75834.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out75565.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out75575.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75716.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: 2s
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Considering the candidate 75388_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75388_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 08:26:20.80 +56:27:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 4.515 1034072475262354560 126.58440550340 +56.46644438374 14.8877 14.0370 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.515#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75389_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75389_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 08:29:24.20 +56:24:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 1.808 1034015545471441408 127.35063945485 +56.40764829936 14.8372 14.3312 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.808#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75394_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75394_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 07:53:27.42 +53:18:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 2.556 984625311352945792 118.36306181031 +53.30215638664 14.1938 13.6453 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.556#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75398_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75398_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 07:40:55.09 +54:18:12.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)
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Considering the candidate 75408_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75408_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 08:33:53.59 +56:23:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 3.878 1034214007320677248 128.47134516126 +56.39836030577 13.8131 13.0500 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.878#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75411_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75411_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 08:19:58.48 +55:53:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 1.831 1033201563269370496 124.99283338898 +55.89071567188 13.2117 12.6843 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.831#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75421_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75421_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 07:40:38.85 +49:30:11.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75450_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75450_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 08:02:15.80 +51:17:43.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.31, MAG_FAINT_SEARCH_LIMIT=12.29)GAIADR2_OUTPUT=# 1.539 935820459801822336 120.56518532945 +51.29519736369 11.9882 11.3016 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.539#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75483_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75483_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 08:08:37.80 +51:32:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75486_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75486_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 08:09:34.51 +55:10:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 1.270 1032920638048649344 122.39319832669 +55.16868007677 12.8313 12.1815 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.270#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75490_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75490_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 08:15:57.81 +50:46:43.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75502_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75502_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 07:45:03.18 +55:43:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.841 985945481221287040 116.26290877619 +55.73127156411 13.1020 12.6302 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.841#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75504_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75504_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 08:01:19.29 +54:26:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75508_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75508_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
Rejecting candidate due to large distance (660.9") between the two second-epoch detections
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Considering the candidate 75509_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75509_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 08:08:33.14 +49:01:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75519_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75519_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 07:50:01.89 +58:23:28.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75522_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75522_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 08:04:38.09 +53:56:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 1.789 1032746017562325632 121.15786710709 +53.94148537496 13.2053 12.6772 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.789#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75525_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75525_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
Rejecting candidate due to large distance (125.8") between the two second-epoch detections
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Considering the candidate 75526_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75526_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 07:41:03.21 +57:04:56.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 75553_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75553_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 08:04:45.83 +53:40:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 0.984 1032733343114806016 121.19063346862 +53.67394477091 13.6575 13.1256 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.984#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75558_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75558_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 07:39:15.39 +52:35:21.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75565_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75565_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 08:09:26.31 +55:11:18.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)
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Considering the candidate 75567_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75567_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 08:17:19.27 +58:59:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 0.271 1083679248747570304 124.33023482036 +58.99081955659 14.0593 13.4458 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.271#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75568_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75568_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 08:28:33.18 +56:48:54.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75573_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75573_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 07:45:34.97 +56:36:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 1.499 1082080421402056320 116.39498074319 +56.61271900580 13.5156 12.8923 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.499#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75575_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
Preparing report for the candidate 75575_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
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Considering the candidate 75578_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75578_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 08:20:27.51 +51:18:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 1.995 1028313649968384512 125.11377624712 +51.30181278862 13.8898 13.3301 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.995#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75599_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75599_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 07:59:02.95 +58:53:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.001 1082739578622795392 119.76249469435 +58.89443706438 14.2341 13.6198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.001#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75606_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75606_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 08:39:52.08 +56:11:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 4.200 1031168325752467968 129.96501944292 +56.18991041837 14.0126 13.5011 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.200#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75616_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
Preparing report for the candidate 75616_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
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Considering the candidate 75647_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75647_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
Rejecting candidate due to large distance (491.9") between the two second-epoch detections
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Considering the candidate 75673_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75673_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 08:11:50.87 +49:33:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 3.980 934679858222110720 122.96073345163 +49.56473134738 14.1797 13.7029 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.980#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75676_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75676_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 07:48:59.55 +56:45:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 2.253 1082050253551660544 117.24842159505 +56.76478440646 14.1841 13.4604 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.253#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75678_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
Preparing report for the candidate 75678_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
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Considering the candidate 75679_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75679_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 08:25:12.07 +54:08:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 1.214 1032101433166233088 126.29972693864 +54.14779515232 14.3360 13.7013 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.214#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75703_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75703_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 08:31:38.24 +49:54:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 1.268 1027167443456435200 127.90923707083 +49.90740214713 14.0804 13.6393 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.268#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75714_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75714_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 07:38:38.62 +57:11:37.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75716_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
Preparing report for the candidate 75716_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
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Considering the candidate 75727_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75727_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
Rejecting candidate due to large distance (106.5") between the two second-epoch detections
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Considering the candidate 75735_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75735_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 08:28:04.98 +58:44:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 2.576 1035482706300500224 127.01942453932 +58.74574698498 14.1464 13.4959 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.576#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75740_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75740_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 08:35:11.43 +51:51:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 0.774 1027802480140492288 128.79744376614 +51.86095532118 14.4811 13.8164 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.774#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75756_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75756_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 07:54:19.53 +52:58:53.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 2.082 984605107826818432 118.58042373640 +52.98150204515 14.2741 13.7787 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.082#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75765_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75765_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 07:48:49.07 +55:26:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 2.494 985149572241672576 117.20341809985 +55.44552556874 14.1302 13.3142 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.494#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75770_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75770_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 08:01:38.00 +55:27:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 1.735 1081025062038385792 120.40748389134 +55.46656419159 14.5680 14.1201 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.735#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75793_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75793_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 08:30:19.60 +54:28:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 3.507 1033578627038303488 127.58011886825 +54.47948624394 14.5689 14.0255 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.507#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75834_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 75834_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 08:24:17.85 +57:48:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 2.254 1034961056752013056 126.07339499323 +57.81062645959 14.9132 14.1902 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.254#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 38213_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 38213_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 07:46:26.36 +48:57:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 3.909 933890133996096640 116.60818006769 +48.96033239529 13.3285 12.5888 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.909#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 39070_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 39070_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 07:45:11.05 +49:06:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 47744_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 47744_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 07:40:25.08 +50:00:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 48804_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 48804_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
Rejecting candidate due to large distance (94.8") between the two second-epoch detections
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Considering the candidate 11108_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 11108_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 07:55:51.17 +57:11:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 48867_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201
The candidate 48867_fd_Lyn-02-Q1b1x1_2026-04-10_03-28-54_20.00sec_-5.00C_LIGHTs_0201 did not pass the final checks