This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 06 17.1557 2461208.6557 13.36 08:32:28.44 +51:19:37.6
167.52297 36.39191 galactic Lyn Second-epoch detections are separated by 2.0" and 6.4 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 | target | 08:32:28.44 +51:19:37.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:32:28.44 +51:19:37.6: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:32:28.44 +51:19:37.6: 16.15 +/- 99.00 upperlimit
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
target,2461208.6557,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260617.1557 13.36CV 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 06 17.1557 2461208.6557 14.73 09:03:37.17 +57:37:18.9
158.90367 40.16421 galactic UMa Second-epoch detections are separated by 5.0" and 5.6 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 | target | 09:03:37.17 +57:37:18.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 09:03:37.17 +57:37:18.9: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 09:03:37.17 +57:37:18.9: 16.02 +/- 99.00 upperlimit
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!
TCP 2026 06 17.1557* 09 03 37.17 +57 37 18.9 14.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461208.6557,14.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260617.1557 14.73CV 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 06 17.1557 2461208.6557 14.62 08:53:47.71 +49:49:00.9
169.26274 39.83581 galactic UMa Second-epoch detections are separated by 3.6" and 6.1 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 | target | 08:53:47.71 +49:49:00.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:53:47.71 +49:49:00.9: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:53:47.71 +49:49:00.9: 16.05 +/- 99.00 upperlimit
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!
TCP 2026 06 17.1557* 08 53 47.71 +49 49 00.9 14.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461208.6557,14.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260617.1557 14.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.73517407 22.02.2026 05:38:29.040 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
First image: 2461093.73517407 22.02.2026 05:38:29.040 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
Last image: 2461208.65595325 17.06.2026 03:44:24.361 /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 0
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.46
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 7177
Objects passed selection criteria: 7172
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: 6225.25
Average stars matched: 6049.75 (97.1808 %)
Memory usage VmPeak: 114016 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jun 16 15:05:04 CDT 2026
VaST build number 1.0rc89-100-g8a7e82c2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Jun 16 22:48:51 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.73517407 22.02.2026 05:38:29.040 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
First image: 2461093.73517407 22.02.2026 05:38:29.040 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
Last image: 2461208.65595325 17.06.2026 03:44:24.361 /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 113
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.15
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 20 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 40316
Objects passed selection criteria: 40244
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 40488.2
Average stars matched: 35831.8 (88.4991 %)
Memory usage VmPeak: 147168 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jun 16 15:05:04 CDT 2026
VaST build number 1.0rc89-100-g8a7e82c2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Jun 16 22:50:42 CDT 2026
Host name: tau
############################################################
######## Processing parameters ########
AAVSO_COMMENT_STRING= NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
ASTCHECK_ASTEROID_SEARCH_RADIUS_ARCSEC=
BAD_REGION_FILE= /var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst
CAMERA_SETTINGS= TTUQ2b1x1
CHECK_POINTING_ACCURACY= yes
DARK_FRAMES_DIR_OR_FILE= /var/www/nmw_calibration/TTUQ2b1x1/darks
EXCLUSION_LIST= ../exclusion_list_TTUQ2.txt
FILTER_BAD_IMG__MAX_APERTURE_STAR_SIZE_PIX= 12.5
FILTER_BAD_IMG__MAX_ELONGATION_AminusB_PIX= 0.55
FILTER_BAD_IMG__MIN_APERTURE_STAR_SIZE_PIX= 2.0
FILTER_BRIGHT_MAG_CUTOFF_TRANSIENT_SEARCH= -5
FILTER_FAINT_MAG_CUTOFF_TRANSIENT_SEARCH= 15.0
FLAT_FIELD_DIR_OR_FILE= /var/www/nmw_calibration/TTUQ2b1x1/flats
FRAME_EDGE_OFFSET_PIX= 600
GAIA_BAND_FOR_CATALOGED_SOURCE_CHECK=
MAX_NEW_TO_REF_MEAN_IMG_VALUE_RATIO= 100
MAX_NEW_IMG_MEAN_VALUE= 25000
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS= 0.18
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS_SOFT_LIMIT= 0.12
MPC_CODE= V36
NMW_CALIBRATION= /var/www/nmw_calibration
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_HARD_LIMIT= 8000
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_SOFT_LIMIT= 4000
OMP_NUM_THREADS=
ONLINE_MPCHECKER_BUTTON_ASTEROID_SEARCH_RADIUS_ARCMIN=
PHOTOMETRIC_CALIBRATION=
REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES= yes
SEXTRACTOR_CONFIG_BRIGHTSTARPASS= default.sex.telephoto_lens_onlybrightstars_v1
SEXTRACTOR_CONFIG_FILES= default.sex.telephoto_lens_onlybrightstars_v1 default.sex.telephoto_lens_vSTL
STARMATCH_RADIUS_PIX= 4
SYSREM_ITERATIONS= 0
TELESCOP=
TELESCOP_NAME_KNOWN_TO_VaST_FOR_FOV_DETERMINATION=
UCAC5_PLATESOLVE_ITERATIONS= 2
FPACK_FULLY_CALIBRATED_IMAGE= no
#######################################
HOSTNAME= tau
USER=
HOME=
#######################################
SExtractor catalog cache: enabled, directory /data_ssd/NMW-TexasTech/vast_sextractor_cache
Reference image directory is set to /data_ssd/NMW-TexasTech/reference_imgs
VIZIER_SITE=vizier.cds.unistra.fr
GAIA_DR2_CLIENT=vizquery (lib/vizquery -> VizieR vizier.cds.unistra.fr)
INFO: MAKE_PNG_PLOTS is set to yes
FITS_FILE_EXT=fits
CALIBRATION_STATUS_PREFIX=
Fields in the data directory:
Lyn-02-Q2b1x1
#######################################
########### Starting Lyn-02-Q2b1x1 ###########
Processing Lyn-02-Q2b1x1
server tau has sufficient free disk space available: 121594 MB at /data_ssd/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 121594 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.png' -> 'transient_report/Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits_preview.png'
Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
renamed 'Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.png' -> 'transient_report/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits_preview.png'
Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
Read-check the input FITS images... read-check OK
Blank image check the input FITS images... blank-image-check OK
Read date check the input FITS images... read-date-check OK
Mean value check the input FITS images... OK, at least two new images have mean values below the threshold.
----------------------------------------------
INFO: REFERENCE_EPOCH__FIRST_IMAGE_MEAN_VALUE= 448.8005
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 561.5627
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 1241.7072
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 487.3530
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 1240.4607
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 486.5334
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 2.76672
INFO: SECOND_EPOCH__SD_ratio= 0.002
----------------------------------------------
Calibration settings: DARK_FRAMES_DIR_OR_FILE=/var/www/nmw_calibration/TTUQ2b1x1/darks FLAT_FIELD_DIR_OR_FILE=/var/www/nmw_calibration/TTUQ2b1x1/flats
EXPTIME = 20.0 / [s] Exposure duration
SET-TEMP= 10.0 / [degC] CCD temperature setpoint
CCD-TEMP= 10.0 / [degC] CCD temperature
FOCTEMP = 27.4799995422363 / [degC] Focuser temperature
AMBTEMP = 27.9 / [degC] Ambient air temperature
No matching dark image found
try_to_calibrate_the_input_frame(): cannot find a good dark frame by running util/find_best_dark.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
EXPTIME = 20.0 / [s] Exposure duration
SET-TEMP= 10.0 / [degC] CCD temperature setpoint
CCD-TEMP= 10.0 / [degC] CCD temperature
FOCTEMP = 27.3600006103516 / [degC] Focuser temperature
AMBTEMP = 27.9 / [degC] Ambient air temperature
No matching dark image found
try_to_calibrate_the_input_frame(): cannot find a good dark frame by running util/find_best_dark.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
after the calibration attempt:
SECOND_EPOCH__FIRST_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
SExtractor catalog cache: saved Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.cat to cache
SExtractor catalog cache: saved Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.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: 2461208.65543993
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits exists and is non-empty
Saving wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits to local_wcs_cache/
'wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits' -> 'local_wcs_cache/wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits'
wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits exists and is non-empty
Saving wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits to local_wcs_cache/
'wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits' -> 'local_wcs_cache/wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits'
wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits exists and is non-empty
Saving wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits to local_wcs_cache/
'wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits' -> 'local_wcs_cache/wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits'
wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits exists and is non-empty
Saving wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits to local_wcs_cache/
'wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits' -> 'local_wcs_cache/wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits (1st reference image)
verification OK: wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
Image size: 927.4'x629.8' 15.5(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.92"/pix along the Y axis
Image center: 08:28:32.338 +53:59:11.90 J2000 4789.000 3195.000
###################################
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits (1st new image)
verification OK: wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
Image size: 937.8'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 08:28:11.222 +53:59:55.95 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:28:32.338 +53:59:11.90
Second-epoch image center 08:28:11.222 +53:59:55.95
Angular distance between the image centers 0.0532 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits (2nd new image)
verification OK: wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
Image size: 937.8'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 08:28:08.268 +54:00:25.54 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:28:32.338 +53:59:11.90
Second-epoch image center 08:28:08.268 +54:00:25.54
Angular distance between the image centers 0.0624 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 08:28:11.222 +53:59:55.95
Second-epoch second image center 08:28:08.268 +54:00:25.54
Angular distance between the image centers 0.01095 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits &> /tmp/tmp.6l5DMuo7pP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits &> /tmp/tmp.qreUpNaGZX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits &> /tmp/tmp.sYYpbAAxIB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits &> /tmp/tmp.y2oNGLAWQl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.wcscat
Found non-empty wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.wcscat
The reference image (wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits) and catalog (wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.wcscat) found
'wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.wcscat' -> 'wcsmag.cat'
Read 10801 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 113.1033 to 142.4919 deg, Dec +47.7238 to +59.2637 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 113.1033 to 142.4919 deg, Dec 47.7238 to 59.2637 deg
Loaded 7240 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): 19 out of 20 total matches.
Matched with Tycho-2 20 out of 10801 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.888000
a=0.000000 b=1.000000 c=22.888000
From vast_summary.log: estimated ref. image limiting mag.: -7.46
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
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 10801 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 113.1033 to 142.4919 deg, Dec +47.7238 to +59.2637 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 113.1033 to 142.4919 deg, Dec 47.7238 to 59.2637 deg
Loaded 7240 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): 19 out of 20 total matches.
Matched with Tycho-2 20 out of 10801 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits:
Forced-photometry filter: calibrated wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits -> calib.txt_param_ref_wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits (aperture=6.3)
Read 10687 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 112.1655 to 141.8814 deg, Dec +48.1871 to +59.2552 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 112.1655 to 141.8814 deg, Dec 48.1871 to 59.2552 deg
Loaded 7092 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): 5067 out of 5264 total matches.
Matched with Tycho-2 5264 out of 10687 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits:
Forced-photometry filter: calibrated wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits -> calib.txt_param_ref_wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits (aperture=6.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
2.4 pix Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits
2.4 pix Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
2.4 pix Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
2.2 pix wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
2.4 pix wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits
Limiting magnitude estimates:
15.4 mag. Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
15.3 mag. Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits
14.7 mag. Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
14.7 mag. Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
All-image limiting magnitude estimate: 14.7 (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.6l5DMuo7pP (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits' -> 'wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
WCS-calibrated image found: wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
Checking if the catalog wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.wcscat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.wcscat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
WCS catalog name: wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=806, passed=10801
Got 10801 stars (including 9985 good ones) from the SExtractor catalog wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.wcscat
util/solve_plate_with_UCAC5 got 10801 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 174 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 143 matched stars entering correct_measured_positions(), 118 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 10.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 138 matched stars entering correct_measured_positions(), 1643 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.92"
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 222 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 203 matched stars entering correct_measured_positions(), 1679 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.77"
Accuracy estimation diagnostic: 201 matched stars entering correct_measured_positions(), 2197 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.14"
Excluding outliers - 201 stars left (next iteration limit 151)
WCS_QUALITY_DIAG: file=Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits N_match=201 sigma_overall_arcsec=11.239 sigma_q1_arcsec=12.826 sigma_q2_arcsec=21.453 sigma_q3_arcsec=9.443 sigma_q4_arcsec=33.388 n_q1=74 n_q2=11 n_q3=108 n_q4=8 worst_quadrant_to_overall_ratio=2.971
The image catalog is written to wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits -region wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.qreUpNaGZX (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_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits' -> 'wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits
WCS-calibrated image found: wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits
Checking if the catalog wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits.wcscat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits.wcscat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits
WCS catalog name: wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=636, passed=10687
Got 10687 stars (including 10043 good ones) from the SExtractor catalog wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits.wcscat
util/solve_plate_with_UCAC5 got 10687 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 10557 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 10558 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 10558 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits N_match=976 sigma_overall_arcsec=0.439 sigma_q1_arcsec=0.340 sigma_q2_arcsec=0.517 sigma_q3_arcsec=0.431 sigma_q4_arcsec=0.461 n_q1=226 n_q2=272 n_q3=225 n_q4=253 worst_quadrant_to_overall_ratio=1.177
The image catalog is written to wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits -region wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.sYYpbAAxIB (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_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.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_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
WCS-calibrated image found: wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
Checking if the catalog wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits.wcscat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits.wcscat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
WCS catalog name: wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=417, passed=6130
Got 6130 stars (including 5706 good ones) from the SExtractor catalog wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits.wcscat
util/solve_plate_with_UCAC5 got 6130 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 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(), 965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 6042 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 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(), 6041 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 6041 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits N_match=974 sigma_overall_arcsec=0.384 sigma_q1_arcsec=0.303 sigma_q2_arcsec=0.419 sigma_q3_arcsec=0.396 sigma_q4_arcsec=0.425 n_q1=226 n_q2=263 n_q3=213 n_q4=272 worst_quadrant_to_overall_ratio=1.107
The image catalog is written to wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits -region wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.y2oNGLAWQl (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_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.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_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
WCS-calibrated image found: wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
Checking if the catalog wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits.wcscat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits.wcscat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
WCS catalog name: wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=417, passed=6152
Got 6152 stars (including 5732 good ones) from the SExtractor catalog wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits.wcscat
util/solve_plate_with_UCAC5 got 6152 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 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(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 6078 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 690 to 748 (Dec 48.1 to 59.3)
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(), 6079 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 6079 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits N_match=974 sigma_overall_arcsec=0.395 sigma_q1_arcsec=0.318 sigma_q2_arcsec=0.431 sigma_q3_arcsec=0.403 sigma_q4_arcsec=0.429 n_q1=226 n_q2=262 n_q3=218 n_q4=268 worst_quadrant_to_overall_ratio=1.092
The image catalog is written to wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits -region wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits sigma_overall=11.239 worst_q_ratio=2.971
ref2=Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits sigma_overall=0.439 worst_q_ratio=1.177
new1=Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits sigma_overall=0.384 worst_q_ratio=1.107
new2=Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits sigma_overall=0.395 worst_q_ratio=1.092
reference average sigma_overall=5.839 worst_q_ratio=2.074
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227_astrometric_residuals.png (201 matched stars from wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 5.98 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207_astrometric_residuals.png (976 matched stars from wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.39 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062_astrometric_residuals.png (974 matched stars from wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063_astrometric_residuals.png (974 matched stars from wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits'
Saving fully-calibrated image wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits'
Preparing the HTML report for the field Lyn-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Lyn-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
SExtractor catalog cache: saved Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.cat to cache
SExtractor catalog cache: saved Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
Creating symlink local_wcs_cache/wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits
Creating symlink local_wcs_cache/wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
Creating symlink local_wcs_cache/wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits exists and is non-empty
wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits exists and is non-empty
wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits exists and is non-empty
wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits (1st reference image)
verification OK: wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
Image size: 927.4'x629.8' 15.5(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.92"/pix along the Y axis
Image center: 08:28:32.338 +53:59:11.90 J2000 4789.000 3195.000
###################################
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits (1st new image)
verification OK: wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
Image size: 937.8'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 08:28:11.222 +53:59:55.95 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:28:32.338 +53:59:11.90
Second-epoch image center 08:28:11.222 +53:59:55.95
Angular distance between the image centers 0.0532 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits (2nd new image)
verification OK: wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
Image size: 937.8'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 08:28:08.268 +54:00:25.54 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:28:32.338 +53:59:11.90
Second-epoch image center 08:28:08.268 +54:00:25.54
Angular distance between the image centers 0.0624 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 08:28:11.222 +53:59:55.95
Second-epoch second image center 08:28:08.268 +54:00:25.54
Angular distance between the image centers 0.01095 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits &> /tmp/tmp.mwJDAbZj7u
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits &> /tmp/tmp.zYwjiqyx9s
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits &> /tmp/tmp.drY5LcUiS9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits &> /tmp/tmp.AhjdYK2dZc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.wcscat
Found non-empty wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.wcscat
The reference image (wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits) and catalog (wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.wcscat) found
'wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.wcscat' -> 'wcsmag.cat'
Read 61028 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 113.0242 to 142.5942 deg, Dec +47.6514 to +59.2748 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 113.0242 to 142.5942 deg, Dec 47.6514 to 59.2748 deg
Loaded 7336 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 22 total matches.
Matched with Tycho-2 22 out of 61028 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.763200
a=0.000000 b=1.000000 c=22.763200
From vast_summary.log: estimated ref. image limiting mag.: -7.15
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.61
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.61
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 61028 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 113.0242 to 142.5942 deg, Dec +47.6514 to +59.2748 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 113.0242 to 142.5942 deg, Dec 47.6514 to 59.2748 deg
Loaded 7336 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 22 total matches.
Matched with Tycho-2 22 out of 61028 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits:
Forced-photometry filter: calibrated wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits -> calib.txt_param_ref_wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits (aperture=4.9)
Read 55363 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 112.0163 to 141.9969 deg, Dec +48.1776 to +59.2644 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 112.0163 to 141.9969 deg, Dec 48.1776 to 59.2644 deg
Loaded 7173 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): 4711 out of 5292 total matches.
Matched with Tycho-2 5292 out of 55363 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits:
Forced-photometry filter: calibrated wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits -> calib.txt_param_ref_wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits (aperture=5.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 62 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
2.3 pix Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits
2.4 pix Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
2.4 pix Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
2.1 pix wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
2.3 pix wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits
Limiting magnitude estimates:
15.6 mag. Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
15.5 mag. Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits
15.0 mag. Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
15.0 mag. Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.mwJDAbZj7u (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits' -> 'wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
WCS-calibrated image found: wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
Checking if the catalog wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.wcscat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.wcscat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
WCS catalog name: wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=3670, passed=61010
Got 61010 stars (including 57216 good ones) from the SExtractor catalog wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.wcscat
util/solve_plate_with_UCAC5 got 61010 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 174 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 141 matched stars entering correct_measured_positions(), 123 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 136 matched stars entering correct_measured_positions(), 9024 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.24"
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 47.6 to 59.3)
Done reading UCAC5 zone files...
Matched 225 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(), 9065 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.19"
Accuracy estimation diagnostic: 204 matched stars entering correct_measured_positions(), 12487 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.57"
Excluding outliers - 204 stars left (next iteration limit 149)
WCS_QUALITY_DIAG: file=Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits N_match=204 sigma_overall_arcsec=10.709 sigma_q1_arcsec=12.482 sigma_q2_arcsec=28.090 sigma_q3_arcsec=8.732 sigma_q4_arcsec=46.768 n_q1=75 n_q2=9 n_q3=115 n_q4=5 worst_quadrant_to_overall_ratio=4.367
The image catalog is written to wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits -region wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.zYwjiqyx9s (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_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits' -> 'wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits
WCS-calibrated image found: wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits
Checking if the catalog wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits.wcscat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits.wcscat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits
WCS catalog name: wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=3142, passed=55344
Got 55344 stars (including 52143 good ones) from the SExtractor catalog wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits.wcscat
util/solve_plate_with_UCAC5 got 55344 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 54652 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 54651 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 54651 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits N_match=976 sigma_overall_arcsec=0.460 sigma_q1_arcsec=0.316 sigma_q2_arcsec=0.527 sigma_q3_arcsec=0.483 sigma_q4_arcsec=0.511 n_q1=226 n_q2=271 n_q3=222 n_q4=257 worst_quadrant_to_overall_ratio=1.145
The image catalog is written to wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits -region wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.drY5LcUiS9 (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_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.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_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
WCS-calibrated image found: wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
Checking if the catalog wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits.wcscat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits.wcscat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
WCS catalog name: wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1909, passed=45966
Got 45966 stars (including 43966 good ones) from the SExtractor catalog wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits.wcscat
util/solve_plate_with_UCAC5 got 45966 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.3)
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(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 44907 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 690 to 748 (Dec 48.0 to 59.3)
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(), 44906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 44906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits N_match=974 sigma_overall_arcsec=0.374 sigma_q1_arcsec=0.303 sigma_q2_arcsec=0.448 sigma_q3_arcsec=0.410 sigma_q4_arcsec=0.380 n_q1=232 n_q2=263 n_q3=219 n_q4=260 worst_quadrant_to_overall_ratio=1.197
The image catalog is written to wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits -region wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.AhjdYK2dZc (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_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.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_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
WCS-calibrated image found: wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
Checking if the catalog wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits.wcscat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits.wcscat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
WCS catalog name: wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=2118, passed=45861
Got 45861 stars (including 43658 good ones) from the SExtractor catalog wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits.wcscat
util/solve_plate_with_UCAC5 got 45861 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 44854 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 44852 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 44851 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits N_match=973 sigma_overall_arcsec=0.382 sigma_q1_arcsec=0.335 sigma_q2_arcsec=0.406 sigma_q3_arcsec=0.409 sigma_q4_arcsec=0.429 n_q1=230 n_q2=255 n_q3=223 n_q4=265 worst_quadrant_to_overall_ratio=1.124
The image catalog is written to wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits -region wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.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_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/wcs_Lyn-02-Q2b1x1_2026-06-16_22-43-40_20.00sec_10.00C_LIGHT_0062.fits
Saving fully-calibrated image wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.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_2026-06-16_CI_Lyn-02-Q2b1x1_224518_TTUQ2b1x1_3835385_VQJLFfLG/wcs_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063.fits
Preparing the HTML report for the field Lyn-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 09:09:02.56 +56:50:37.1: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 09:07:50.30 +56:46:23.3: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:38:40.78 +56:31:42.5: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 09:02:42.47 +55:20:09.6: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:19:15.85 +49:45:54.2: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:04:37.07 +53:57:40.7: 16.22 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:59.69 +55:44:45.3: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 09:13:40.20 +54:28:21.5: 14.03 +/- 0.05 detection
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:09:21.58 +54:07:53.3: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 09:09:21.57 +57:23:22.1: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 09:09:02.56 +56:50:37.1: 13.95 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.06
Forced photometry filter REJECTED candidate at 09:09:02.56 +56:50:37.1: ref_mag=13.95 +/- 0.06 new_mean_mag=13.9597 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 09:07:50.30 +56:46:23.3: 14.36 +/- 0.08 detection
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:38:40.78 +56:31:42.5: 14.64 +/- 0.09 detection
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 09:02:42.47 +55:20:09.6: 14.11 +/- 0.06 detection
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:59.69 +55:44:45.3: 14.65 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.36 +/- 0.08
Forced photometry reference-image weighted average: 14.64 +/- 0.09
Forced photometry filter REJECTED candidate at 09:07:50.30 +56:46:23.3: ref_mag=14.36 +/- 0.08 new_mean_mag=14.3490 delta=0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:38:40.78 +56:31:42.5: ref_mag=14.64 +/- 0.09 new_mean_mag=14.3338 delta=0.31 (need > 0.90)
Forced photometry reference-image weighted average: 14.11 +/- 0.06
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:19:15.85 +49:45:54.2: 14.19 +/- 0.06 detection
Forced photometry filter REJECTED candidate at 09:02:42.47 +55:20:09.6: ref_mag=14.11 +/- 0.06 new_mean_mag=14.2216 delta=-0.11 (need > 0.90)
Forced photometry reference-image weighted average: 14.65 +/- 0.09
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:09:21.58 +54:07:53.3: 14.24 +/- 0.06 detection
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 09:13:40.20 +54:28:21.5: 14.04 +/- 0.06 detection
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:04:37.07 +53:57:40.7: 14.49 +/- 0.08 detection
Forced photometry filter REJECTED candidate at 08:22:59.69 +55:44:45.3: ref_mag=14.65 +/- 0.09 new_mean_mag=14.5305 delta=0.12 (need > 0.90)
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 09:09:21.57 +57:23:22.1: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.19 +/- 0.06
Forced photometry reference-image weighted average: 14.24 +/- 0.06
Forced photometry reference-image weighted average: 14.03 +/- 0.04
Forced photometry reference-image weighted average: 14.49 +/- 0.08
Forced photometry filter REJECTED candidate at 08:19:15.85 +49:45:54.2: ref_mag=14.19 +/- 0.06 new_mean_mag=14.1053 delta=0.08 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:09:21.58 +54:07:53.3: ref_mag=14.24 +/- 0.06 new_mean_mag=14.1760 delta=0.06 (need > 0.90)
Forced photometry reference-image weighted average: 13.80 +/- 0.05
Forced photometry filter REJECTED candidate at 09:13:40.20 +54:28:21.5: ref_mag=14.03 +/- 0.04 new_mean_mag=14.1289 delta=-0.10 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:04:37.07 +53:57:40.7: ref_mag=14.49 +/- 0.08 new_mean_mag=14.6477 delta=-0.16 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:09:21.57 +57:23:22.1: ref_mag=13.80 +/- 0.05 new_mean_mag=14.2409 delta=-0.44 (need > 0.90)
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:24:36.10 +56:01:00.3: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:38:34.93 +54:34:59.5: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:09:08.03 +56:50:15.8: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:35:03.88 +54:49:05.0: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:17:24.24 +55:07:15.2: 16.29 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:29:36.12 +50:55:11.4: 16.22 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:33:57.46 +54:02:43.1: 16.29 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:37:27.86 +50:42:02.8: 16.28 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:13:19.55 +49:42:07.3: 16.16 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:38:34.93 +54:34:59.5: 13.79 +/- 0.04 detection
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:35:03.88 +54:49:05.0: 13.14 +/- 0.02 detection
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:17:24.24 +55:07:15.2: 13.64 +/- 0.03 detection
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:29:36.12 +50:55:11.4: 12.37 +/- 0.01 detection
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:24:36.10 +56:01:00.3: 14.13 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.04
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:09:08.03 +56:50:15.8: 13.64 +/- 0.04 detection
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:33:57.46 +54:02:43.1: 14.37 +/- 0.06 detection
Forced photometry filter REJECTED candidate at 08:38:34.93 +54:34:59.5: ref_mag=13.79 +/- 0.04 new_mean_mag=13.5783 delta=0.21 (need > 0.90)
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:37:27.86 +50:42:02.8: 13.63 +/- 0.04 detection
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:13:19.55 +49:42:07.3: 12.71 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 08:35:03.88 +54:49:05.0: ref_mag=13.14 +/- 0.02 new_mean_mag=13.2052 delta=-0.07 (need > 0.90)
Forced photometry reference-image weighted average: 13.64 +/- 0.03
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Forced photometry reference-image weighted average: 14.13 +/- 0.05
Forced photometry filter REJECTED candidate at 08:17:24.24 +55:07:15.2: ref_mag=13.64 +/- 0.03 new_mean_mag=13.6325 delta=0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:29:36.12 +50:55:11.4: ref_mag=12.37 +/- 0.01 new_mean_mag=12.1548 delta=0.21 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:24:36.10 +56:01:00.3: ref_mag=14.13 +/- 0.05 new_mean_mag=13.9575 delta=0.17 (need > 0.90)
Forced photometry reference-image weighted average: 13.64 +/- 0.04
Forced photometry reference-image weighted average: 14.37 +/- 0.06
Forced photometry reference-image weighted average: 13.63 +/- 0.04
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Forced photometry filter REJECTED candidate at 08:09:08.03 +56:50:15.8: ref_mag=13.64 +/- 0.04 new_mean_mag=13.7411 delta=-0.10 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:33:57.46 +54:02:43.1: ref_mag=14.37 +/- 0.06 new_mean_mag=13.9984 delta=0.37 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:37:27.86 +50:42:02.8: ref_mag=13.63 +/- 0.04 new_mean_mag=13.2748 delta=0.35 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:13:19.55 +49:42:07.3: ref_mag=12.71 +/- 0.02 new_mean_mag=12.7881 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 09:07:25.23 +52:22:55.5: 12.98 +/- 0.02 detection
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 09:07:25.23 +52:22:55.5: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Forced photometry filter REJECTED candidate at 09:07:25.23 +52:22:55.5: ref_mag=12.45 +/- 0.01 new_mean_mag=12.5819 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:32:28.44 +51:19:37.6: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:32:28.44 +51:19:37.6: 16.15 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:29:56.45 +55:10:58.1: 16.30 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 09:03:37.17 +57:37:18.9: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:29:56.45 +55:10:58.1: 14.22 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.06
Forced photometry filter REJECTED candidate at 08:29:56.45 +55:10:58.1: ref_mag=14.22 +/- 0.06 new_mean_mag=14.0780 delta=0.15 (need > 0.90)
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:42:47.39 +54:02:28.8: 14.10 +/- 0.05 detection
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:53:47.71 +49:49:00.9: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 09:03:37.17 +57:37:18.9: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:42:47.39 +54:02:28.8: 14.92 +/- 0.12 detection
Forced photometry on wcs_Lyn-02-Q2b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:53:47.71 +49:49:00.9: 16.05 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.23 +/- 0.05
Forced photometry filter REJECTED candidate at 08:42:47.39 +54:02:28.8: ref_mag=14.23 +/- 0.05 new_mean_mag=14.7341 delta=-0.51 (need > 0.90)
Adding exclusion_list_local.txt__out75600.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80965.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 22s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 74125_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 74125_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
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Considering the candidate 74127_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 74127_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
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Considering the candidate 74128_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 74128_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
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Considering the candidate 74133_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 74133_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
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Considering the candidate 74134_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 74134_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
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Considering the candidate 74139_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 74139_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
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Considering the candidate 74141_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 74141_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
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Considering the candidate 74145_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 74145_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
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Considering the candidate 74146_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 74146_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
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Considering the candidate 74150_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 74150_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
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Considering the candidate 74153_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 74153_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
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Considering the candidate 74157_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 74157_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
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Considering the candidate 74159_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 74159_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
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Considering the candidate 74160_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 74160_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
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Considering the candidate 74161_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 74161_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
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Considering the candidate 74162_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 74162_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
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Considering the candidate 74163_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 74163_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
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Considering the candidate 74168_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 74168_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 08:20:03.48 +51:48:19.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74172_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 74172_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
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Considering the candidate 74173_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 74173_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
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Considering the candidate 74707_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 74707_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 08:18:09.65 +54:10:19.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 74952_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 74952_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
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Considering the candidate 74966_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 74966_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 08:08:37.58 +51:32:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74971_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 74971_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 08:15:57.61 +50:46:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75326_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 75326_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 08:01:19.04 +54:26:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75443_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 75443_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 08:34:56.82 +50:29:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75600_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
Preparing report for the candidate 75600_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
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Considering the candidate 75685_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 75685_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 75711_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 75711_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 08:51:52.97 +58:08:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75833_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 75833_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 08:25:37.19 +52:15:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75842_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 75842_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 08:13:22.59 +52:32:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75880_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 75880_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 08:39:01.76 +52:57:17.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 75946_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 75946_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 08:20:27.40 +51:18:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75953_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 75953_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 08:04:45.63 +53:40:27.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76017_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 76017_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 76231_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 76231_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 08:09:26.15 +55:11:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76354_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 76354_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 76476_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 76476_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 76683_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 76683_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 08:25:11.88 +54:08:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76742_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 76742_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 08:32:20.78 +53:06:39.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 76819_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 76819_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
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Considering the candidate 77062_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 77062_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 77275_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 77275_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 77326_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 77326_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
**** FOUND 08:30:19.14 +54:28:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77667_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 77667_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 78257_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 78257_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 78351_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 78351_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 78399_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 78399_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 78513_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 78513_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 78611_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 78611_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 78805_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 78805_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 78835_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 78835_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 78877_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 78877_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 79461_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
Preparing report for the candidate 79461_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
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Considering the candidate 80023_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 80023_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 80578_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 80578_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 80665_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 80665_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
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Considering the candidate 80965_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
Preparing report for the candidate 80965_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
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Considering the candidate 81261_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 81261_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 19082_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 19082_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (38.7") between the two second-epoch detections
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Considering the candidate 33806_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 33806_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (39.8") between the two second-epoch detections
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Considering the candidate 47319_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063
The candidate 47319_Lyn-02-Q2b1x1_2026-06-16_22-44-24_20.00sec_10.00C_LIGHT_0063 did not pass the final checks
